The galaxy presents a generally smooth appearance with a bright central bulge. There is a hint of a disk-like structure, though it is not clearly defined and appears relatively featureless. The galaxy is elongated, possibly indicative of a spheroid or elliptical morphology rather than a spiral. The color profile suggests an older stellar population with a predominantly yellow-orange hue. There are no apparent signs of recent major mergers or strong tidal disturbances, though minor disturbances cannot be ruled out. The lack of bright blue regions suggests a low star formation rate. The galaxy's morphology appears to be transitioning from a disk galaxy to an elliptical galaxy, or could just be an elliptical galaxy that is slightly misshapen. The central bulge dominates the overall light profile.
