The galaxy presents as a primarily smooth object, exhibiting an elliptical morphology with a high degree of roundness. There is a minor indication of a possible, subtle disturbance in the galaxy's structure, potentially a minor tidal interaction, as there appears to be a slight asymmetry in the distribution of its light. There is no significant central bulge or distinct spiral arm structure. The galaxy appears relatively quiescent, suggesting a low star formation rate. The color profile indicates that the galaxy is dominated by older stellar populations, exhibiting redder colors, thus suggesting a later-type galaxy. There may be a very faint halo surrounding the galaxy.
