The target galaxy presents as a spiral type, exhibiting distinct spiral arm structures. The arms display a medium to loose winding, tracing a prominent pattern outwards from the central region. Two spiral arms are clearly discernible. The central bulge appears to be moderate in size, contributing significantly to the galaxy's overall luminosity. A barred structure is evident, extending across a noticeable portion of the central region, exhibiting characteristics of a strong to weak bar. There are signs of a major disturbance or interaction, possibly indicating a merging event is in progress. The overall color gradient suggests a mix of stellar populations, with a bluer hue along the outer spiral arms, potentially indicating active star formation, and a yellower, older stellar population concentrating within the bulge. The galaxy is not seen edge-on. There does not appear to be a dominant smooth component.
