The galaxy appears to be an elliptical type, exhibiting a smooth, concentrated light profile that diminishes gradually with increasing radial distance from the center. The central region is noticeably brighter and more compact, suggesting a significant concentration of stars or possibly an active galactic nucleus. The overall shape approximates a circular morphology with minimal discernible substructure or spiral arm features. Color gradients across the galaxy are subtle, but there is a slight tendency towards redder hues in the central bulge, potentially indicating an older stellar population. The outer regions exhibit a bluer tint. There does not appear to be any interaction with another galaxy or significant tidal debris. The galaxy shows no signs of being actively disturbed or undergoing a major merger event. The estimated size of this galaxy is about 4.5 kpc, making it a relatively small galaxy.
