This galaxy appears to be a relatively smooth, lenticular or early-type spiral galaxy, possibly at an intermediate redshift. It exhibits a generally elliptical morphology, appearing somewhat elongated but not strongly disc-like. The galaxy's color profile suggests a dominant older stellar population, with a redder hue in the optical bands indicating diminished recent star formation. There are no strong indications of spiral arms or prominent dust lanes, consistent with a smoother morphological classification. There appears to be no evidence of major disturbances or ongoing merging activity, though minor tidal interactions cannot be completely ruled out. Based on its apparent size and overall characteristics, it appears to be a moderate-sized galaxy, but further spectroscopic or photometric redshift measurements are needed to properly constrain its intrinsic properties.
