The galaxy appears to be a relatively smooth, elliptical structure. It exhibits a bright, centrally concentrated bulge that dominates its overall luminosity. The galaxy appears mostly uniform in color, displaying a yellowish hue, indicative of an older stellar population with lower levels of active star formation. There is little evidence of spiral arms or dust lanes, suggesting a lack of significant cold gas reservoirs. The galaxy’s shape is close to circular, with a slight suggestion of elongation. There are no obvious signs of major mergers or significant tidal disturbances in the immediate vicinity of the galaxy.
