The galaxy presents as a generally smooth, elliptical object with a slight elongation. The light profile appears centrally concentrated. There is a radial color gradient, appearing yellower in the central region, suggesting an older stellar population towards the core. The outer regions appear bluer, potentially indicating more recent star formation. There is no discernible spiral structure or evidence of a prominent disk. There may be a very slight distortion in the isophotes, potentially indicating a minor interaction or past merger event, though no significant tidal features are visible. The overall color and morphology suggest a relatively massive galaxy.
