The galaxy presents as a relatively smooth, elliptical morphology, though the elongation suggests a possible transition towards a lenticular type. Its color index indicates a predominantly older stellar population, with a yellow-red hue dominating its overall appearance. The light distribution appears concentrated towards the center, with a gradual decrease in brightness towards the outer regions. There is little evidence of distinct spiral arm structures or prominent dust lanes. There are no clear signs of ongoing major mergers or tidal disruptions, however, a small disturbance cannot be ruled out. The galaxy appears to be a non-star forming galaxy, meaning it is a quiescent galaxy.
