The galaxy presents as a roughly elliptical, highly concentrated object with a smooth, symmetrical profile. The central region exhibits a bright, orange-yellow hue, suggesting an older stellar population dominated by redder stars. Moving outward from the core, the color transitions to a slightly greenish-yellow, potentially indicating the presence of some younger stars or a small amount of ongoing star formation, though at a very low rate. There is no discernible spiral arm structure or bar. The galaxy appears relatively undisturbed with no obvious signs of a recent major merger or tidal interactions. A subtle elongation is visible, contributing to its lenticular appearance. The overall morphology is consistent with an early-type galaxy, likely an elliptical or lenticular galaxy, with an estimated mass range typical for galaxies of this type.
