The galaxy presents as a somewhat smooth, concentrated distribution of light. There is a bright, unresolved central region, possibly indicative of an active galactic nucleus or a dense stellar population. The overall shape is close to circular in projection, with only minor deviations from perfect symmetry. Fainter, diffuse light extends outward from the core, gradually fading into the background. There is a slight color gradient visible, with the central regions appearing subtly yellower than the outer parts, suggesting a difference in stellar populations or dust content between the core and the surrounding regions. There are no clearly defined spiral arms, bar structures, or prominent dust lanes visible within the galaxy's image. Based on its morphology, it could be classified as an elliptical or lenticular galaxy. Signs of recent major merger events are not obvious.
