The galaxy presents as a relatively smooth, centrally concentrated object with a high degree of roundness. A prominent bulge dominates the galaxy's morphology, exhibiting a bright, yellowish hue. This indicates a population of older, likely metal-rich stars. Fainter, diffuse bluish light surrounds the central bulge, suggesting the presence of a stellar disk and some ongoing, but likely low, levels of star formation. No distinct spiral arms or bar structures are readily apparent. The overall structure appears undisturbed, with no signs of major mergers or significant tidal interactions.
