The galaxy presents as a slightly elongated, cigar-shaped system. The light distribution appears relatively smooth and concentrated, with a subtle color gradient transitioning from a bluer hue at the edges to a subtly redder core. There is little to no evidence of spiral arm structure or prominent dust lanes. The overall appearance suggests a disk galaxy viewed at a high inclination, though the smoothness of the light profile is more indicative of a lenticular (S0) or early-type spiral. There is no visually apparent merging or tidal disturbance. Star formation is present but very little, mostly within the disk.
