The galaxy presents a somewhat elliptical morphology, displaying a flattened disk structure. Its color profile indicates a bluer central region, possibly suggesting ongoing or recent star formation activity. There's a notable central bulge, which appears to be a significant component of the galaxy's overall structure, though the extent and prominence is moderate.

The disk appears to be the dominant feature, exhibiting evidence of faint spiral arm structures. No significant tidal disturbances or signs of major mergers are readily apparent in the galaxy's morphology, although subtle asymmetries might suggest minor interactions. The overall light distribution is relatively smooth, which is consistent with the appearance of a relatively normal disk galaxy at the observed resolution.
