The galaxy presents a largely smooth morphology. It exhibits an elliptical shape, appearing more elongated than circular, with a subtle cigar-like form.  There appears to be a central bulge region which is brighter and more concentrated than the surrounding galactic disk.  The overall color suggests a population of older stars, potentially indicating a relatively low current star formation rate. There is no obvious spiral structure visible. There is a possible minor disturbance detected via a faint arm-like structure extending from the main body of the galaxy on one side, however, overall, there is no indication of it undergoing a major merging event.
