The galaxy presents as a somewhat elliptical structure, appearing more elongated than circular. The central region exhibits a concentrated, bright core with a yellowish hue, suggesting an older stellar population. Moving outward from the core, the color transitions to a slightly bluer shade, potentially indicating the presence of younger stars or ongoing star formation, though it does not appear very pronounced. The galaxy appears relatively smooth in texture, with only subtle indications of spiral arms or prominent dust lanes, it is likely a galaxy that has exhausted a good amount of its star-forming fuel. There is no obvious sign of any major mergers. 
