The galaxy appears as a single, largely featureless object with a smooth light profile. The morphology is generally elliptical, displaying a high degree of circular symmetry. There is a slight color gradient across the galaxy, with a somewhat more reddish hue in the central region compared to the outer edges, suggesting older stellar populations are more concentrated toward the center, and a higher fraction of younger stars is concentrated in the outer regions. There is no evidence of spiral arms, a central bar, or other distinct morphological features. The galaxy may be actively forming stars, and is relatively massive. No significant tidal disturbances or merging activity is apparent, but a slight disturbance cannot be ruled out.
