The galaxy exhibits an overall elliptical morphology with a high degree of central concentration. The light distribution appears relatively smooth with a lack of prominent spiral arm structures or distinct features. There is a slight elongation. The core region displays a bright yellowish-orange hue, suggestive of an older stellar population. The outer regions transition to a more diffuse, bluish color profile which might indicate some, albeit limited, ongoing star formation activity. No signs of major mergers or tidal disturbances are apparent from its structure, though it appears to have possibly undergone a minor disturbance in the past. The roundness is somewhere in between completely round and more elongated. Overall, the galaxy appears to be a fairly massive system, with a relatively low specific star formation rate.
