The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated, bright central bulge, grading outward to a less luminous halo. The galaxy appears to be largely featureless, lacking any distinct spiral arms or prominent dust lanes within the image resolution. The color gradient transitions from a yellowish-white core to a bluer outer region, potentially indicative of a varied stellar population with a mix of older and younger stars. There may be some indication of minor disturbances or interactions but that is not conclusive. The apparent shape suggests a mostly relaxed morphology, likely not undergoing any major mergers or significant starburst activity at the time of observation.
