The galaxy presents as a largely featureless elliptical object. Its morphology appears smooth and relatively rounded, lacking any distinct spiral arms or prominent disk-like structures. The light distribution is centrally concentrated, with a gradual decrease in luminosity towards the outer regions. There is a slight asymmetry, but no clear signs of ongoing major merging activity or tidal disturbances are observed, though minor disturbances cannot be ruled out. The galaxy's color index indicates a redder population, suggestive of an older stellar population and potentially lower rates of ongoing star formation. Overall, the galaxy seems to be a typical, passively evolving elliptical galaxy at a low redshift.
