The galaxy presents as a centrally concentrated, relatively smooth, and symmetrical object. It exhibits an elliptical morphology, appearing generally rounded in shape with a slight elongation. A bright central bulge dominates the galaxy's luminosity, decreasing in intensity towards the outer regions. There is some evidence of faint, diffuse material extending beyond the main body of the galaxy, but no distinct spiral arm structure or prominent dust lanes are visible. A subtle color gradient is discernible, with the central region appearing more yellow-orange, potentially indicating an older stellar population, while the outer regions exhibit a slightly bluer hue. No signs of ongoing major mergers are directly observed in the image. However, there is evidence of a potential minor disturbance or tidal feature on one edge of the galaxy. Overall, the galaxy appears to be a massive, evolved system with relatively low levels of current star formation.
