The galaxy presents as a relatively smooth, disk-like structure. The light profile appears centrally concentrated, exhibiting a bulge component with a yellowish hue. This suggests an older stellar population dominates the nuclear region. The outer disk region appears fainter and bluer, potentially indicating ongoing star formation, although this is not immediately obvious from the image. There is no clear evidence of spiral arm structure or a bar feature. The galaxy shows hints of minor disturbances, but it seems to be relatively isolated without any major merging events.
