The galaxy presents a somewhat elliptical morphology, displaying a smooth, centrally concentrated light profile. A distinct, brighter, yellowish core region is apparent, suggesting an older stellar population or possibly the presence of an active galactic nucleus. Diffuse, fainter light extends outward from this central core. 

There appears to be evidence of a possible interaction or merger event in its past. The overall structure is notably disturbed, indicating gravitational interaction with a nearby galaxy. This disturbance could imply ongoing or recent tidal effects. While the majority of the galaxy appears smooth, there is a small region that is less symmetrical. 

Given its color and smooth structure, the galaxy likely contains primarily older stars and exhibits a low rate of star formation.
