The galaxy presents as a relatively smooth, elliptical object. It exhibits a high degree of central concentration, with light intensity decreasing gradually from the core. The overall shape is close to circular, indicating minimal apparent flattening. There is subtle evidence of possible minor tidal disturbances or interactions, with slight asymmetries observable. The red color suggests an older stellar population, potentially indicating relatively low current star formation activity. It also appears that the galaxy could potentially be merging or interacting with another galaxy nearby. 
