The galaxy presents a generally smooth morphology, although some disturbances are visible. The object appears nearly circular, with a slightly irregular shape. A bright central core or bulge region is present. The color profile suggests a relatively high fraction of young stars or active galactic nucleus activity within the central region, with a color suggesting increased intensity in the blue-green wavelengths. Possible minor tidal disturbances appear evident in its outer regions, possibly indicating an ongoing or recent minor merger. The object's light distribution is concentrated in the central region, gradually decreasing toward the edge of the galaxy, showing faint and diffuse structures.
