The galaxy presents a generally smooth, elliptical morphology. The core exhibits a bright, concentrated luminosity profile, suggesting a high density of stars in the central region. Moving outwards from the core, the light gradually fades into a more diffuse halo. The galaxy appears largely featureless with no obvious spiral arm structures, bars, or dust lanes visible in the image. It exhibits a subtly elongated shape, deviating slightly from a perfectly circular form. The color profile shows a dominant yellow-red hue, particularly concentrated in the core, indicative of an older stellar population. Fainter blue tinges are observed in the outer regions, potentially hinting at some ongoing, albeit limited, star formation activity. The overall appearance is consistent with a mature galaxy, likely with a substantial stellar mass, undergoing a relatively quiescent period. No signs of significant disturbances or ongoing major mergers are discernible.
