The galaxy presents as a relatively smooth, elliptical-like structure. A concentrated central bulge exhibits a yellowish-orange hue, suggesting an older stellar population dominated by evolved stars. Moving outward from the core, the galaxy fades gradually, displaying a bluer color gradient. Faint and ill-defined spiral arm-like extensions or features are tentatively visible, hinting at the possibility of a weak disk component. The overall morphology is largely undisturbed, with no obvious signs of ongoing major mergers or strong tidal interactions. There is a very slight asymmetry observed, with one side being slightly more extended than the other. The galaxy is relatively compact.
