The galaxy exhibits an overall elliptical morphology, appearing largely smooth with minimal discernible structure. Its core is characterized by a bright, concentrated luminosity, which fades gradually towards the outer regions. The color gradient suggests a redder hue in the central region, potentially indicating an older stellar population, while the outer regions appear bluer, possibly indicative of ongoing or recent star formation activity. There is a slight asymmetry in the galaxy's profile, possibly suggestive of a minor gravitational interaction or disturbance. Given the estimated size and morphology, this galaxy could be classified as an early-type galaxy undergoing some level of star formation.
