The galaxy presents as a smooth, elongated object. Its overall form is quite regular, exhibiting a cigar-like shape. The central region displays a yellowish hue, suggestive of an older stellar population. Progressing outwards from the core, a subtle shift towards bluer tones is discernible. There is no strong evidence of spiral arm structures or significant dust lanes. The galaxy appears relatively undisturbed with no obvious signs of recent major merger activity.
