The galaxy exhibits a prominent disk structure, suggesting it's a spiral or lenticular type. Distinct spiral arm features are discernible, though somewhat flocculent. A central bulge is present, though it appears to be relatively small in comparison to the overall galaxy size. The disk appears to be at a slight angle relative to our line of sight, but is still largely face-on. There's no apparent bar structure. The galaxy's color suggests active star formation is present, particularly within the spiral arms. No signs of ongoing major merging events are obvious, though there may be evidence of minor tidal disturbances or interactions. The galaxy presents an overall smooth appearance.
