The galaxy appears as a centrally concentrated, smooth object with a faint, diffuse halo. The primary structure is a flattened ellipsoid. It exhibits a slight elongation, appearing somewhat cigar-shaped in its overall form. No distinct spiral arms or prominent dust lanes are discernible. The galaxy's color is generally bluish-white in the core, transitioning to slightly redder hues in the outer regions. This color gradient might indicate a population of younger, hotter stars concentrated in the central region, with older, cooler stars dominating the outskirts. The absence of significant morphological disturbances suggests the galaxy is relatively undisturbed and not currently undergoing major merging activity, although there may be some evidence of a minor interaction in its past.
