The galaxy appears as a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution suggests an older stellar population, with a yellowish-orange hue dominating the core, gradually fading into a more reddish color toward the outer regions. There is no discernible spiral arm structure or significant dust lane obscuration visible in this image. The galaxy exhibits a somewhat regular, rounded shape, showing no indications of major mergers or tidal disturbances. Any present star formation is likely occurring at a very low rate.
