The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The core exhibits a yellowish hue, potentially indicating an older stellar population. The outer regions of the galaxy fade into a bluer color, suggesting the presence of younger, hotter stars, though this is less pronounced. There is a lack of distinct spiral arm structure or significant dust lanes. The galaxy appears somewhat elongated, deviating slightly from a perfect circular shape. No signs of major tidal disturbances or ongoing merger events are immediately apparent, though a subtle asymmetry cannot be ruled out. The overall impression is that of a mature galaxy with a dominant bulge component and a relatively smooth, featureless disk.
