The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a centrally concentrated luminosity profile, fading gradually towards the edges. The color is predominantly yellowish-white, suggesting a stellar population dominated by older, evolved stars, though there appears to be hints of bluer regions possibly near the core or along the disk of the galaxy. There's no indication of prominent spiral arms or significant dust lanes. The galaxy's overall shape is closer to a rounded form, rather than being elongated or cigar-shaped. There's no visually obvious evidence of on-going major merger events.
