The galaxy presents as a largely smooth, elliptical object. A bright, concentrated central bulge dominates the morphology, gradually fading into a more diffuse halo. The galaxy exhibits a slight elongation, deviating minimally from a perfectly circular shape. There is no readily apparent spiral arm structure or distinct dust lane features visible in this imaging. The color profile suggests a population of older stars, with a subtle shift towards redder hues from the core to the outer regions, indicating potential variations in stellar population age or metallicity. No signs of ongoing major merging events or significant tidal disturbances are evident, suggesting a relatively isolated and dynamically stable system. Faint, subtle irregularities in the outer halo may indicate minor past interactions or accretion events.
