The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that transitions smoothly outward, with no readily apparent spiral arms or distinct features. The overall color profile suggests a population dominated by older stars, given the subtle reddish-yellow hue. There's a slight elongation observed, deviating from a perfectly circular morphology. No significant tidal features or signs of major merger events are immediately visible, although subtle disturbances cannot be ruled out at this resolution.
