The galaxy presents as a somewhat elongated, likely disk-shaped structure. It exhibits a yellowish-red hue, which may indicate an older stellar population or significant dust obscuration. There appears to be a central bulge region that is brighter and more concentrated than the surrounding disk. There is little indication of spiral arm structure. The galaxy appears relatively undisturbed, with no obvious signs of ongoing major merger activity or tidal distortions. The shape is in between round and cigar shaped, leaning towards cigar shaped. The disk is not the prominent feature.
