The galaxy presents an elongated, cigar-like morphology. The central region exhibits a brighter, yellowish-orange hue, suggestive of an older stellar population. This central concentration gradually diffuses outwards into a less defined, bluer halo. The overall structure appears relatively smooth, with no prominent spiral arms or distinct dust lanes visible. The extended halo indicates a possible flattened disk galaxy. There is little evidence of active galactic nuclei activity in the central region of the galaxy.
