The galaxy presents as an elongated, cigar-shaped system. A smooth, centrally concentrated bulge dominates the morphology, exhibiting a color gradient towards a redder hue in the innermost region, suggestive of an older stellar population. Moving outward from the bulge, the galaxy shows a faint, disk-like structure. The disk appears relatively featureless with subtle color variations. Blue tinges are interspersed throughout the outer regions, possibly indicating areas of recent or ongoing star formation, albeit at a low rate. There is no obvious spiral arm structure, suggesting a disk that is relatively undisturbed. No strong tidal features or signs of a major merger are apparent; however, some minor asymmetry or irregularities could be present in the disk. The galaxy exhibits a moderate amount of light, indicating an intermediate luminosity for a system at its distance. Overall, it appears to be a relatively quiescent disk galaxy with a prominent bulge and weak star formation.
