The galaxy presents as a moderately bright, elliptical or lenticular structure. It exhibits a smooth, relatively featureless morphology, lacking any prominent spiral arms or significant dust lanes visible in this image. The central bulge appears moderately concentrated and exhibits a yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy fade gradually into the background, indicating a diffuse halo. The overall shape deviates slightly from perfect circularity, with a suggestion of elongation, possibly indicating a transition from a more spherical elliptical type to a disk-like lenticular morphology. There is no obvious evidence of ongoing major mergers or tidal disturbances, although a subtle asymmetry may indicate a minor interaction history. The blue color index suggests that there may be some presence of on-going star formation.
