The galaxy presents as an elliptical morphology, appearing largely smooth and featureless. The light profile is concentrated towards the center, with a gradual decrease in intensity outwards, suggesting a well-established stellar population. The core region exhibits a slightly redder hue than the outer regions, which could be due to a higher concentration of older stars and dust extinction towards the center. The bluer color observed in the outer areas possibly indicates the presence of younger, hotter stars. The overall shape appears quite rounded. There is no discernible evidence of tidal features or major disturbances, indicating a lack of recent major merger activity. Faint, diffuse light extends outwards from the main body of the galaxy, possibly representing a sparse halo population.
