The galaxy presents as a fairly smooth, rounded structure with a concentrated central bulge. There is a slight elongation suggesting it is not perfectly spherical, but appears mostly elliptical in shape. The core of the galaxy exhibits a yellowish-orange hue, indicating an older stellar population. There appears to be some asymmetry, possibly due to a minor interaction, or perhaps just internal variations in stellar density. A small region just to the west of the central core appears slightly redder than the rest of the galaxy, potentially suggesting a region of dust obscuration or a population of evolved red giants. The galaxy appears relatively undisturbed with no apparent strong tidal features or evidence of a major merger event.
