The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The overall color appears slightly reddish, suggesting a population of older stars. There is a lack of distinct spiral arm features or prominent dust lanes. The galaxy exhibits an elongated shape, appearing somewhat cigar-shaped. There does not appear to be a strong presence of active star formation, with the galaxy's light dominated by an older stellar population. There is no obvious major merging activity, although a slight asymmetry or minor disturbance cannot be entirely ruled out. The galaxy possesses a moderate degree of central concentration.
