The galaxy presents a generally smooth morphology, with a cigar-shaped appearance. The central region exhibits a concentrated bulge, displaying a yellowish-white hue, suggestive of an older stellar population. Extending outwards from the core is a faint disk structure. Hints of bluer tones are seen at the edges of the galaxy, hinting at the presence of younger stars and regions of active star formation. There are no obvious signs of a major merger. The galaxy's overall form suggests that it is likely a disk galaxy viewed at an oblique angle.