The galaxy presents a relatively smooth morphology, with a dominant central bulge. It shows a flattened, disk-like structure, although the disk itself is not well-defined. The galaxy exhibits a blue hue, which suggests the presence of younger stellar populations and ongoing star formation, although the star formation rate appears to be low. No strong spiral arm features are apparent, although some faint and ill-defined features within the disk suggest a disrupted morphology. There is some evidence of minor tidal disturbances or potential interaction. The overall shape of the galaxy appears to be somewhere in between round and cigar-shaped.
