The galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated bulge with a gradual decrease in luminosity towards the outer regions. There is a slight elongation, though the overall shape is mostly rounded, with no obvious spiral arm structure or prominent dust lanes visible. The galaxy presents a yellowish hue, likely indicative of an older stellar population and low current star formation activity. No signs of recent major merger events are apparent from the image. It does not show any substantial irregularities or tidal tails.
