The galaxy presents as an elliptical morphology, exhibiting a high degree of smoothness. The central bulge is prominent and appears nearly spherical, with a concentrated brightness profile. A faint, diffuse halo surrounds the central region, gradually fading into the background sky. A slight asymmetry is observed, with a subtle extension or possible tidal feature extending from the main body. The overall color profile suggests an older stellar population, consistent with a relatively quiescent star formation rate. The galaxy appears relatively isolated, with no obvious signs of ongoing major merger activity, however there may be signs of minor disturbance. There may be a second object associated with it on the lower left side of the galaxy.
