The galaxy presents a largely smooth, elliptical morphology. It appears predominantly featureless, lacking strong indications of spiral arms or a prominent disk structure. The light profile suggests a concentrated central bulge that gradually fades into the outer regions. The central region has a slightly reddish hue, possibly indicating an older stellar population. The outer areas appear bluer, hinting at a younger population of stars. There are no obvious signs of major tidal disturbances or ongoing mergers. The overall shape appears close to round. The estimated size places it within the range of typical galaxies. It seems the galaxy is actively forming stars, though potentially at a moderate rate.
