The galaxy presents as a well-defined, elongated structure, suggestive of a disk galaxy seen at an oblique angle. The central bulge is prominent, exhibiting a yellowish-white hue, indicative of an older stellar population. Moving outwards from the bulge, a fainter, bluish disk is observed. The color gradient suggests ongoing star formation within the disk, albeit at a moderate rate. The overall morphology indicates the galaxy does not show signs of any major disturbances or ongoing mergers, it appears to be relatively quiescent. The structure appears smooth overall, with no obvious spiral arm structure visible at this resolution. The light distribution suggests a flattened, cigar-shaped structure. The angular size suggests that the galaxy is a moderate-sized object.
