The galaxy appears to be a relatively compact system, exhibiting a smooth, elliptical morphology. The core region is characterized by a bright, concentrated luminosity, suggestive of an older stellar population. A gradual decrease in light intensity is observed moving outward from the center, transitioning into a fainter, diffuse halo. No distinct spiral arm structures or prominent dust lanes are apparent. The overall color profile suggests a more evolved galaxy with limited ongoing star formation, as evidenced by the lack of significant blue emission associated with young, hot stars. There are no obvious signs of major tidal disturbances or interactions with other galaxies.
