The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated luminosity profile, suggesting a bulge-dominated morphology. The galaxy presents an elongated shape, deviating from a perfectly circular form. There is a noticeable color gradient, with the core region appearing yellower or redder compared to the outer regions, which show a bluer tint. This color difference potentially indicates differing stellar populations, with older, redder stars concentrated in the center and younger, bluer stars more prevalent in the outer regions. No prominent spiral arms or obvious signs of ongoing major mergers are detected in this image. There is no obvious dust lane present.