The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that gradually fades into a diffuse halo. The core displays a yellowish-orange hue, suggestive of an older stellar population dominating the nuclear region. The outer regions are bluer in color, indicating the potential presence of younger stars or ongoing star formation, though at a low rate. There is no apparent spiral structure or significant dust lanes visible. The galaxy exhibits a slightly elongated shape, approaching round, rather than a highly flattened or cigar-shaped morphology. No obvious signs of tidal interactions or recent merger events are apparent from the image.
