The galaxy appears as a relatively smooth, elliptical structure. There is a bright, concentrated central bulge exhibiting a yellowish hue, which likely indicates a population of older, redder stars. Fainter, diffuse extensions surround the core, gradually fading into the background sky. The overall shape is close to circular, with no obvious signs of spiral arms or significant dust lanes. There are no indications of ongoing major merging activity. The subtle color gradients suggest variations in stellar populations across the galaxy, but without higher resolution imaging, a detailed analysis of star formation regions is not possible.
