The galaxy exhibits a clear elongated, cigar-like morphology. The central region displays a bright, concentrated bulge with a yellowish-white hue, suggesting an older stellar population. Extending outward from the bulge is a fainter, bluer disk component. The blue color suggests the presence of ongoing star formation within the disk, although the overall star formation rate appears relatively low. The disk is not uniformly smooth; there are subtle indications of spiral arm structures, though they are not highly defined. The galaxy appears relatively isolated, with no obvious signs of major interaction or merging events. There is a slight asymmetry present within the disk structure, potentially indicative of a minor disturbance or previous interaction. Overall, this galaxy likely represents a disk galaxy undergoing a relatively quiescent evolutionary phase.
