The galaxy presents as a luminous, centrally concentrated object with a smooth overall morphology. The central region exhibits a yellowish hue, suggestive of an older stellar population. The galaxy is elongated, displaying a somewhat cigar-shaped appearance. There's evidence of a faint, diffuse disk component surrounding the central bulge. The disk appears to be subtly disturbed, possibly indicating minor gravitational interactions. The system does not appear to be undergoing a major merger event. There is possible evidence of a weak tidal tail extending away from the main body. The overall color profile suggests moderate star formation activity.
