The galaxy presents as a primarily smooth and elliptical morphology. It exhibits a centrally concentrated light profile, with a gradual decline in surface brightness outward from the core. There is a slight elongation in its shape, though it appears closer to round than cigar-shaped. The overall color index suggests the presence of an older stellar population. While there are no prominent tidal features or indications of a recent major merger event, there may be a subtle asymmetry suggesting a minor interaction or disturbance in its past. The rate of star formation appears low based on the color.
