The galaxy presents as a primarily smooth, elliptical-shaped structure, exhibiting a concentration of light towards its center. There is a gradual decline in luminosity from the core outwards, with no evident spiral arm structures or prominent dust lanes. The color profile indicates a generally older stellar population, potentially with a diminished rate of recent star formation. The morphological classification suggests it is likely a relatively undisturbed system, with no significant signs of an ongoing major merger. There is, however, a very slight indication of a possible minor tidal disruption, which could be the result of a minor interaction, although this is not entirely clear. Overall, the galaxy appears to be a relatively quiescent, evolved system.
