The galaxy presents as a relatively smooth, elliptical-like structure, elongated with a cigar shape. The light profile appears centrally concentrated, fading gradually towards the edges. There is a noticeable color gradient within the galaxy. The central region displays a redder hue, potentially indicating an older stellar population. The outer regions show a bluer color, possibly indicative of younger stars or ongoing star formation, but at low levels. There are slight disturbances or features present indicating potentially minor interactions. The galaxy exhibits no obvious spiral arms, bars, or other prominent disk features. Overall, it gives the impression of a mature galaxy, with indications of more recent, but limited, star formation activity.
