This galaxy exhibits a flattened, disk-like morphology, indicative of a spiral or lenticular type. The structure shows a central bulge region that appears relatively small compared to the overall extent of the galaxy. Two very prominent spiral arms originate from this bulge region, one being noticeably shorter than the other. These spiral arms are well-defined, suggesting ongoing or recent star formation activity. The distribution of light within the galaxy is not uniform. Patches of bluer light indicate regions of increased star formation, while redder light suggests areas of older stellar populations. The galaxy does not appear to be undergoing any major interactions or merging events, although there may be some minor disturbances present.
