The galaxy appears to be an elliptical or lenticular type. It exhibits a generally smooth light distribution with a bright, concentrated central bulge. There is no clear evidence of spiral arms or significant dust lanes. The galaxy has a slightly elongated shape. A notable feature is the presence of what appears to be a tidal tail, suggesting a past or ongoing merger event. The galaxy displays a bluish hue in the central region, potentially indicating some recent star formation activity. The overall color is indicative of a galaxy dominated by older stellar populations.
