The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. The morphology suggests a spheroid-dominated system, lacking prominent spiral arms or a distinct disk. There is a slight elongation, but the overall shape is fairly circular. The color profile indicates a yellow/white hue towards the core, possibly suggesting an older stellar population. The outer regions fade into a blue hue, which may indicate the presence of younger stars. There is no evidence of ongoing major mergers or significant tidal disturbances in the image.
