The galaxy presents as a primarily smooth, elliptical object with a slight elongation along a vertical axis. The central region exhibits a concentrated, bright core, suggesting the presence of a significant stellar population or perhaps an active galactic nucleus, though definitive determination requires spectroscopic data. A fainter, somewhat detached region is observed inferior to the main galaxy, suggestive of either a smaller, interacting galaxy or tidal debris resulting from a past merger event. The color profile indicates a predominantly older stellar population, with a yellow-red hue dominating the central region, consistent with evolved stars. There is little indication of ongoing star formation. Overall, the galaxy appears to be a relatively massive, early-type system undergoing or having undergone some form of interaction.
