The galaxy presents a relatively smooth, elliptical morphology. Its light profile exhibits a concentrated central bulge, surrounded by a more diffuse halo. The color is generally consistent, though slightly redder in the central regions. There's a suggestion of asymmetry in the outer halo, but no clear indication of a major merger event or significant tidal disturbances. The apparent absence of spiral arms or strong dust lanes suggests a lower rate of ongoing star formation. The object appears relatively compact, but its luminosity suggests a substantial mass.
