The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge with a yellowish hue, suggesting a population of older stars. The overall shape appears largely spheroidal with little to no presence of defined spiral arms or a discernible disk. There is a slight elongation visible, but it is minimal, leading to a classification of predominantly round. No major disturbances or signs of ongoing mergers are readily apparent in the image, however, there is evidence of possible tidal interactions with smaller galactic bodies. The color profile indicates a lack of significant recent star formation, supported by the yellowish light which suggests an older stellar population throughout the galaxy.
