The galaxy presents as a centrally concentrated, elliptical morphology with a smooth light distribution. There is a distinct, bright core that diminishes in intensity outwards. The ellipticity is moderate, appearing somewhat flattened. No spiral arm structures or significant dust lanes are discernible within the image resolution. The overall color appears to be redder, suggestive of an older stellar population. The galaxy exhibits a well-defined spheroidal shape, with a gradual decrease in luminosity away from the nucleus, indicative of a high Sersic index. There is no obvious evidence of recent major merger activity or significant tidal disturbances. The galaxy does not appear to have any pronounced features such as star-forming regions or irregularities in its structure.
