The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a bright, concentrated luminosity profile, indicative of a substantial stellar population and potentially an active galactic nucleus. The shape is more of a rounded in-between shape than distinctly round or cigar-shaped. There is no clear evidence of spiral arm structure or a prominent disk component. Faint, diffuse extensions are barely discernible at the periphery, possibly representing a halo of older stars or tidal debris from past interactions, but no major or minor mergers. Its red color suggests a high degree of stellar maturity.
