The galaxy appears to be a relatively smooth, elliptical-type galaxy with a dominant central bulge. The light distribution indicates an absence of prominent spiral arms or distinct features within the disk. The overall color is somewhat redder, suggesting a population of older stars and potentially lower ongoing star formation. The galaxy exhibits a slightly elongated shape, deviating modestly from perfect circularity. There is no clear evidence of tidal tails, strong distortions, or other indications of major recent merger activity. The galaxy is likely a massive system, with a significant stellar mass. Current star formation activity is suspected to be relatively low. There may be some minor disturbance present.
