The galaxy presents as a lenticular or early spiral type, viewed at an oblique angle. A bright, concentrated central bulge dominates the morphology, exhibiting a yellowish-white color profile indicating a population of older stars. Surrounding the bulge, a faint, diffuse disk is discernible, displaying a bluer hue suggestive of ongoing star formation. The disk appears somewhat asymmetrical, potentially indicative of tidal interactions or recent merger events. There are subtle irregularities in the disk's structure, possibly signifying minor disturbances. The overall impression is that of a galaxy undergoing intermediate levels of star formation activity, with morphological features suggesting a complex evolutionary history.
