The galaxy presents as a smooth, elliptical morphology. The light distribution is concentrated centrally with a gradual decline outwards, suggesting a high Sersic index, indicative of an older stellar population. The color profile exhibits a radial gradient, appearing more yellow-white towards the core and trending towards redder hues at the periphery. The ellipticity is notable, with a major to minor axis ratio indicating a flattened spheroid. There is no evidence of spiral arm structures, dust lanes, or active star-forming regions based on its color. The smoothness of the light profile suggests that it's a relaxed system, and is not a merging system. Overall, the galaxy likely is a relatively massive system with minimal star formation, and comprised mostly of older stars.