The object appears to be a spiral galaxy of moderate angular size. The disk shows some texture but appears to have a fairly smooth light distribution overall, potentially indicating an older stellar population or a relatively face-on orientation that obscures detailed features. There are some signs of minor disturbances, such as slight asymmetries in the spiral arms, which suggests possible interaction with a smaller object or internal dynamic processes. There is no strong evidence for ongoing major merging activity. The color appears somewhat red, possibly indicating moderate redshift or a significant population of older, redder stars. There is a very weak bulge apparent, which is almost indistinguishable from the disk light distribution.
