The galaxy presents a generally smooth and rounded morphology. The central region exhibits a bright, concentrated luminosity, appearing yellow-white in color. The outer regions appear to gradually fade, exhibiting a fainter, mottled appearance. Faint red emissions are observed on one side of the galaxy, possibly indicating areas of ongoing star formation or dust extinction. There is no discernible evidence of spiral arms, a prominent disk structure, or significant tidal disturbances indicative of recent major merger events. The overall structure suggests a system dominated by an older stellar population, with relatively suppressed star formation.
