The galaxy presents a slightly irregular morphology. A central, brighter region suggests the presence of a bulge, although it appears relatively diffuse rather than sharply defined. Extending from this central region is a fainter, somewhat asymmetric disk. There's a hint of bluer colors within the disk, possibly indicating regions of recent star formation. Overall, the galaxy appears relatively low in mass and exhibits a low star formation rate. Some degree of disturbance is possible, with a likelihood of a minor interaction or internal irregularity contributing to the asymmetry in the disk and the diffuse nature of the bulge. The light distribution is not uniformly smooth and the overall shape is not perfectly elliptical.
