The galaxy presents as a flattened, ellipsoidal structure, suggesting a classification leaning towards an elliptical or lenticular type. The light distribution appears relatively smooth, with a concentration towards the center indicative of a central bulge. The color profile suggests a population of older stars, displaying a yellow-red hue across the galaxy. No distinct spiral arms or prominent dust lanes are visible. The galaxy's elongation implies a possible rotation axis perpendicular to our line of sight. There's no evident sign of tidal interactions or major mergers. The galaxy shows an intermediate roundness shape, between round and cigar shaped. The galaxy presents with no major disturbances. Based on the overall morphology, the galaxy seems to be relatively evolved and stable.
