The galaxy exhibits a moderate level of structural complexity. It appears to be primarily a spiral galaxy, though with some indications of a possible recent or ongoing interaction or minor merger. The primary body of the galaxy presents a relatively smooth appearance with only hints of defined spiral arms, suggesting a flocculent or disturbed morphology. The central bulge appears indistinct and is not strongly pronounced. A slight asymmetry is present in the distribution of light, possibly indicative of tidal disturbances or past interactions. The overall color is somewhat blue, potentially signifying ongoing star formation activity in the disk, but it is not overly pronounced, indicating the star formation rate may be moderate. There are subtle variations in color across the galaxy's body, suggesting different stellar populations are distributed throughout. Based on its apparent size, it is likely a reasonably sized galaxy, neither particularly large nor particularly small.
