The galaxy presents an overall elongated, cigar-like morphology. A centrally concentrated bulge region exhibits a strong red-orange color gradient, suggesting an older stellar population or significant dust obscuration. Fainter, bluer light extends from the central bulge region, indicating the presence of more recent star formation in a disk component. There is no clear indication of spiral arms or a bar structure. The galaxy appears relatively isolated, although there are hints of a minor disturbance or interaction in the outer regions.
