The galaxy presents a largely smooth and elliptical morphology. Its central region exhibits a bright, concentrated luminosity, suggesting a significant stellar density or active galactic nucleus. The light distribution falls off gradually from the core, transitioning to a fainter halo or extended envelope. There's minimal evidence of spiral arm structure or significant dust lanes; the galaxy appears primarily spheroidal. There is a very slight asymmetry, suggestive of possible minor interaction or tidal disturbance. Overall, the galaxy's appearance implies an evolved system with diminished star formation activity.