The galaxy presents as a roughly elliptical structure, with a dominant central bulge. There is a slight elongation, suggesting it is not perfectly spherical, more of a lumpy football shape.

The color gradient indicates a central concentration of older stars. Overall light is slightly yellowish in the center, shifting toward a bluer hue in the outer regions. This suggests there may be a small amount of ongoing star formation, or possibly an older population in the central region. 

No distinct spiral arms are visible. Overall, the galaxy exhibits a relatively smooth appearance, with some signs of minor disturbance. There may be an indication of a recent minor merger event, causing some distortions in the outer regions.