The galaxy presents as a relatively smooth, elliptical-like structure with a bright central core. There is a distinct color gradient observed from the center outwards. The core exhibits a yellow-orange hue, indicative of an older stellar population dominated by red giant stars, or significant dust obscuration. Moving outwards, the light becomes slightly bluer, suggesting the presence of some younger, hotter stars within the galaxy, especially in the area to the upper right of the core. There appears to be a close proximity to another smaller source. It is not clear if this is an object behind or in front of the primary galaxy, or if it is a sign of tidal disturbance. Given its round appearance, high smoothness and lack of spiral arms, it is likely that the galaxy is an elliptical type. There may be ongoing or recent star formation, although the rate seems to be quite low. The estimated size suggests it is a fairly large galaxy.
