The galaxy exhibits a pronounced elongated, cigar-like morphology. It presents a smooth overall appearance, with minimal indication of spiral arm structure. The color profile suggests a relatively evolved stellar population, leaning towards redder wavelengths. This observation potentially corresponds to decreased levels of ongoing star formation. The morphology is also suggestive of a possible S0 galaxy, exhibiting characteristics of both spiral and elliptical galaxies. There is no indication of major disturbances or a clear merging event, although the slight asymmetry may indicate a minor interaction history.
