This galaxy appears to be an intermediate spiral galaxy with a slightly disturbed morphology. The central bulge exhibits a moderate degree of roundness. The spiral arms are not well-defined, appearing somewhat flocculent and exhibiting signs of tidal disruption. There is evidence of ongoing or recent minor merger activity. The galaxy displays a broad range of stellar populations, from younger, bluer regions associated with star formation to older, redder populations in the bulge. Overall, the galaxy suggests an active evolutionary history involving interactions with other galaxies.
