The galaxy presents as a centrally concentrated object with a smooth, largely featureless morphology. It exhibits a generally elliptical or spheroidal shape, appearing mostly round. The light distribution suggests a bulge-dominated system, with a gradual decrease in brightness outward from the core. Color gradients appear subtle, perhaps indicating a relatively uniform stellar population or a lack of significant dust extinction. There is no obvious evidence of spiral arms, bars, or tidal features, suggesting it is likely a relaxed system without ongoing major mergers or interactions. The absence of distinct blue regions implies a low star formation rate.
