The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a noticeable elongation, displaying a cigar-like morphology rather than a perfectly circular appearance. The color profile suggests a predominantly older stellar population, leaning towards redder wavelengths with hints of yellow in its core. There is no obvious spiral arm structure or significant dust lane obscuration visible. It displays no evidence of major ongoing merger activity or significant tidal disturbances, appearing relatively undisturbed in its immediate environment. Star formation is likely low.
