The galaxy presents as a fairly smooth, elliptical-like structure. The central bulge appears prominent, with a concentrated bright yellowish hue, indicating a population of older stars. Moving outwards from the core, the color gradually fades with the light becoming dimmer with what appear to be some areas of possible diffuse dust. There is no clear evidence of spiral arms or a distinct disk structure. The overall shape appears moderately rounded, though perhaps slightly elongated. There are no obvious signs of any ongoing major mergers or significant tidal disturbances. There is a small amount of blue hinting at recent star formation, but not much.