The galaxy presents as an elliptical morphology, likely exhibiting a relatively smooth overall structure with low rates of star formation. It appears moderately bright. The light distribution indicates a high degree of central concentration, possibly with a prominent bulge. Evidences of mergers or tidal disturbances can be observed, suggesting past or ongoing interactions with another galaxy. The central region exhibits a yellowish hue, likely indicating an older stellar population. The galaxy exhibits a faint, red color in the nucleus, possibly indicating that the galaxy is in the process of merging with another.
