The galaxy presents as a roughly elliptical object, exhibiting a centrally concentrated light profile with a relatively smooth appearance. There is little evidence of spiral arm structure or distinct dust lanes. The color gradient suggests a predominantly older stellar population, with bluer hues concentrated toward the galactic core. A subtle elongation is noticeable, deviating from a perfectly circular morphology. The outer regions of the galaxy appear less well-defined, fading gradually into the background sky. There is no obvious sign of ongoing major mergers or tidal disturbances, but a faint asymmetry is noticeable which could possibly indicate a minor disturbance. Overall, the galaxy appears to be a relatively quiescent system.