The galaxy presents as a slightly elongated structure, appearing roughly disk-shaped in projection. It exhibits a bright, concentrated central region, possibly indicative of a bulge or active galactic nucleus. Surrounding this central concentration is an extended, fainter disk. There appear to be some indications of structural irregularities or disturbances within the disk, although these are subtle. There may be some hints of spiral arm structure present, but it is not well-defined. The overall color profile shows a shift towards bluer hues in the outer regions of the disk, potentially suggesting ongoing star formation. The galaxy appears to be relatively isolated, without any obvious major merging events occurring, though minor tidal disturbances cannot be ruled out.
