The galaxy presents as a relatively small, elliptical or lenticular system at a redshift of approximately 0.096, indicating a substantial distance. It exhibits a smooth, centrally concentrated light profile, with a noticeable lack of distinct spiral arm structures. The core region appears to be somewhat brighter, possibly indicative of an active galactic nucleus or a higher density of stars in the galactic bulge. The overall shape is moderately elongated. The color indices suggest a relatively old stellar population, with a predominance of redder hues. There does not seem to be evidence of active star formation or significant dust lanes within the visible spectrum.
