The galaxy presents as a singular, relatively smooth object. The central region exhibits a concentrated, bright core, suggesting a high stellar density. The light profile appears to gradually decrease in intensity from the center outwards, without any obvious spiral arm structures or prominent dust lanes visible at this resolution. The overall shape appears mostly round, with no distinct elongation. Coloration leans towards yellow/orange, potentially indicating an older stellar population and a lower rate of ongoing star formation. There is no obvious evidence of tidal disturbances, major mergers, or significant ongoing interactions with other galaxies.
