The galaxy presents as a somewhat elliptical structure, with a notable central bulge that appears relatively smooth and concentrated. Moving outwards from the central bulge, there's an indication of a disk component, though it appears somewhat disturbed or irregular. Faint, diffuse features extend from the main body, hinting at possible tidal interactions or minor disturbances. The color profile suggests the presence of both older stellar populations (towards the redder end) and some regions of ongoing star formation, inferred from the bluer hues. The overall morphology could be classified as an intermediate type, exhibiting characteristics of both elliptical and spiral galaxies, but with notable irregularities.
