This galaxy presents as an elliptical system, viewed at a significant angle. The light distribution suggests a centrally concentrated morphology, with a smooth, diffuse halo extending outwards. The core appears relatively bright and yellowish, possibly indicating a population of older stars. Moving outwards, the galaxy displays a gradual decrease in luminosity. The overall color profile, with the redder center, suggests a lack of significant ongoing star formation, further implying an older stellar population dominating the galaxy's structure. There does not appear to be any spiral structure or dust lanes visible in this image. The smooth, relatively featureless appearance suggests that the object is unlikely to be undergoing a major merger or significant tidal interaction.
