The galaxy presents a generally smooth and rounded morphology, exhibiting characteristics of an elliptical or lenticular galaxy. The light distribution is centrally concentrated, with a gradual decrease in intensity towards the outer regions. A slight elongation is noted, with its overall appearance being close to round. There are no strong indications of spiral arms or prominent features. A noticeable color gradient is observed, with the central region appearing more yellowish-red compared to the outer areas, which exhibit a bluish-green hue. This color difference suggests that the core may contain an older stellar population. The absence of significant dust lanes or prominent star-forming regions supports the classification of the galaxy as an early-type galaxy with minimal ongoing star formation. However, a considerable fraction of the light appears to come from younger stars as suggested by the blue color. There are indications of a minor merger having happened recently. The central region does show signs of minor disturbances and asymmetry, indicating the possibility of interactions with other galaxies or recent merger events.
