The galaxy presents as a predominantly elliptical morphology, exhibiting a smooth, concentrated central bulge that diminishes in intensity towards the outer regions. The color profile indicates a bias towards older stellar populations, evidenced by the yellowish-red hue dominating the central region, which then fades to a slightly bluer edge on one side. There is a slight asymmetry to the galaxy, with what might be a faint, diffuse arm-like extension on its right side. No distinct dust lanes or spiral arm structures are discernible, however, it does appear as though there is some sort of interaction or disruption going on, indicated by the color change on the right side. This galaxy seems to be relatively evolved, with little active star formation visible.
