The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, with light gradually decreasing in intensity outwards. The color profile appears largely consistent across the galaxy, tending towards redder wavelengths. This suggests a stellar population dominated by older, less massive stars, and relatively low levels of ongoing star formation. The shape appears nearly circular, with no obvious signs of a disk-like component or significant tidal disturbances or mergers. Based on its morphology, it is consistent with being a spheroidal galaxy.
