The galaxy appears to be an elliptical type, exhibiting a largely smooth and featureless morphology. Its light profile suggests a centrally concentrated bulge, indicated by the yellowish hue, which gradually diffuses outwards into a fainter halo. There is some suggestion of a possible disk-like component, evidenced by a slight flattening or extension in one direction. Color gradients across the galaxy indicate varying stellar populations, with the central regions being dominated by older, redder stars and bluer colors towards the outer edges. The galaxy may be undergoing some minor disturbances. These disturbances seem to be a result of an ongoing minor or major merger. The galaxy’s estimated size is approximately 6 kpc.