The galaxy presents as a primarily smooth, elliptical-shaped structure with a concentrated central bulge exhibiting a yellowish hue, suggesting an older stellar population dominating this region. The light profile appears relatively uniform, without prominent spiral arms or significant dust lanes visible. The galaxy displays a slight elongation, deviating minimally from a perfectly circular shape. There is no indication of ongoing major merger events or strong tidal disturbances in the immediate vicinity based on its morphology. The color gradient observed suggests a potential decrease in stellar age and/or metallicity from the center outwards, with the outer regions exhibiting slightly bluer tones, though this is subtle. The overall impression is that of a relatively evolved, quiescent galaxy with a substantial stellar mass.