This galaxy presents a primarily smooth morphology, appearing largely elliptical in shape with a degree of roundness. The central region exhibits a bright, concentrated luminosity, indicative of a substantial stellar population or active galactic nucleus. Fainter, diffuse extensions emanate from the core, contributing to a surrounding halo. There are subtle indications of potential disturbances, suggesting a possible minor interaction or ongoing merger event. Overall, the galaxy appears to be in a relatively late stage of its evolution, with a substantial mass and moderate star formation activity. The color profile suggests the presence of both older stellar populations in the core and younger, star-forming regions in the outer areas, implying that the galaxy's star formation history may have been ongoing in recent epochs.
