The galaxy appears to be an elliptical type, characterized by a generally smooth and featureless morphology. The light distribution suggests a centrally concentrated bulge, with a gradual decrease in luminosity towards the outer regions. The overall shape deviates slightly from perfectly round, appearing somewhat elongated. There is no obvious evidence of spiral arms or a prominent disk structure. There are no obvious signs of on-going or recent major merger activity. The color profile displays a slight reddish hue, especially within the central bulge, indicative of an older stellar population and reduced star formation activity. Faint blue regions appear in the outer areas, pointing to the presence of areas with lower levels of recent star forming regions.
