The galaxy presents as a relatively smooth, elliptical morphology, although some subtle features suggest a possible disk component. The central bulge exhibits high luminosity, with a gradual decrease in surface brightness moving outward towards the edges. The shape is more of an intermediate elliptical rather than perfectly circular or elongated. There is no evidence of significant merging activity or major disturbances in the galaxy's structure; however, there is some very minor irregularity to the galaxy. The size of the galaxy is relatively small. Given the color profile, the galaxy likely contains a population of older stars, indicating a suppressed star formation rate. Overall, the galaxy exhibits characteristics consistent with a quiescent system undergoing limited current star formation.
