The galaxy presents a largely smooth and rounded morphology. The central region exhibits a yellowish-white hue, suggesting a population of older stars. A subtle blue halo surrounds the core, potentially indicating ongoing, though not vigorous, star formation. No distinct spiral arms or bar structures are readily discernible. The overall appearance suggests an elliptical galaxy, possibly with a faint, diffuse disk component. There is no obvious evidence of any major mergers or tidal disturbances.
