The galaxy presents an elliptical morphology, appearing largely spheroidal with a smooth light distribution. There is a prominent central bulge characterized by a concentrated luminosity, suggesting a high stellar density in this region. The overall color index indicates a redder hue, hinting at an older stellar population and a relatively low rate of ongoing star formation. Although the image resolution limits detailed analysis, there is a subtle indication of a surrounding halo or extended envelope of stars, but there is no apparent spiral arm structure or significant dust lane obscuration. Minor asymmetric features may be present, suggesting potential interactions or past mergers.
