This galaxy presents a face-on spiral structure with discernible arm features. There is some visual indication of distortion, possibly due to interactions or internal dynamics. The central bulge is compact and relatively small compared to the disk component. Star formation appears to be ongoing within the spiral arms. A moderate amount of blue light is present, suggesting the presence of younger stellar populations associated with ongoing star formation. The overall luminosity indicates this is a galaxy of moderate size. There may be evidence of an interaction on one side of the galaxy, with less prominent arms that appear to be more diffuse. Overall, this seems to be an actively star-forming galaxy undergoing morphological evolution.
