The galaxy presents as a generally smooth, elliptical structure. Its core exhibits a bright, concentrated luminosity, appearing yellowish-orange, suggesting a population of older stars. The galaxy gradually fades towards its outer edges. The shape appears more elongated, with an axis ratio suggestive of an E4-E5 elliptical morphology. There is no obvious disk-like structure. Minimal visual evidence of spiral arms or significant dust lanes is present. Faint, slightly bluer outer regions may indicate some ongoing, albeit low-level, star formation. There are no apparent signs of major mergers or tidal disturbances, though subtle asymmetries cannot be entirely ruled out at this resolution. The galaxy appears relatively isolated, without obvious companion galaxies nearby.
