The galaxy presents as a centrally concentrated system with a relatively smooth and homogenous light distribution. It appears elliptical in shape, exhibiting a high degree of circularity. The core region demonstrates a bright, compact profile, suggestive of a high stellar density. Moving outward, the galaxy gradually decreases in surface brightness. There is no apparent spiral arm structure or dust lane obscuration. A subtle blue hue is present, indicating the presence of a younger stellar population. However, the dominant color profile appears more consistent with evolved stars, trending towards the redder end of the spectrum. There are no obvious signs of tidal disturbances or interactions with other galaxies in the immediate vicinity. Overall, the galaxy's features are indicative of a mature, relatively quiescent system dominated by an older stellar population.
