The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology. Its overall shape is approximately elliptical, with a slight deviation towards a more elongated form. The light profile suggests a relatively even distribution of stars, with the highest concentration located within the core region. 

The color of the galaxy is predominantly yellow-orange, indicating a stellar population dominated by older, redder stars. There is a slight color gradient observable, with the core region appearing more yellow and the outer regions trending toward a more orange hue. This may suggest differences in stellar populations or metallicity between the center and the outskirts. 

There is no clear evidence of distinct spiral arms or prominent dust lanes. A faint irregular structure is visible to one side of the core and could potentially indicate a minor interaction or disturbance.
