The galaxy presents as a flattened, elongated structure, suggestive of a disk galaxy viewed at a high inclination. There is a central bulge, exhibiting a somewhat amorphous morphology. The overall color profile indicates a bias towards older stellar populations. The spiral arms, if present, are tightly wound, and not easily distinguishable. The edges of the galaxy appear smooth, with no indication of significant tidal disturbances or ongoing major mergers. There is a slight asymmetry in the brightness distribution, with a subtle suggestion of minor interaction. Overall the galaxy's morphology is likely transitioning to an early-type spiral.
