The galaxy presents as a relatively smooth, elliptical morphology. Its color profile appears generally redder, suggestive of an older stellar population and reduced star formation activity. The light distribution is concentrated towards the central region, with a gradual fading outwards. Two apparent objects are visible extending from the central region of the galaxy, implying that it is experiencing either minor disturbance due to an ongoing merging event, or potentially star forming regions that are being illuminated by the central area.
