The galaxy presents an overall smooth morphology, suggestive of an elliptical or lenticular type. There is a noticeable elongation, with the galaxy appearing cigar-shaped, and a general lack of distinct spiral arm structures or prominent features. The central region exhibits a bright, concentrated luminosity, indicating a likely bulge component. The color gradient suggests a predominantly older stellar population, with a yellowish or reddish hue dominating the core. Fainter, bluer regions appear at the outer edges, possibly indicating ongoing, though subdued, star formation. There is no strong evidence of major mergers or significant tidal disturbances.
