The galaxy presents a generally smooth, elliptical morphology. It displays a concentrated central bulge that dominates the overall luminosity. The light is most intense in the core, gradually diminishing toward the outer edges. The color profile of this galaxy exhibits a noticeable gradient. The core appears yellowish-white, which potentially indicates an older stellar population. The outer regions show a faint greenish-blue tint. The galaxy lacks prominent spiral arms or dust lanes, further supporting the classification of an elliptical galaxy. There is no evidence of ongoing major mergers, although there might be faint hints of tidal disturbances. Overall, the galaxy appears to be an evolved system with a dominant old stellar population.