The galaxy presents as a concentrated spheroid of light, with a dominant, relatively uniform color profile consistent with older stellar populations. It lacks a clear spiral structure or defined dust lanes. The morphology appears generally smooth, with an elliptical shape that leans towards round. There are no obvious signs of ongoing major merger events, although a slight asymmetry in the light distribution suggests the possibility of a minor interaction or disturbance. The relatively red color suggests low star formation activity. A smaller companion galaxy is present nearby, and appears as a smaller, less luminous system with a more irregular, elongated morphology and bluer color suggesting some star forming activity.
