The galaxy presents as a centrally concentrated, luminous object with a smooth morphology. Its overall shape appears roughly elliptical, with a gradual decrease in luminosity from the core outwards. The color profile exhibits a yellowish-red hue, suggesting a population of older stars. There is no apparent evidence of spiral arm structure or significant dust lanes. Minor irregularities or faint tidal features may be present, but the resolution is insufficient to confirm. The galaxy appears relatively isolated, without any clear signs of ongoing major mergers or strong gravitational disturbances. Star formation activity is likely low, indicated by the galaxy's color.
