The galaxy presents as a relatively smooth, disk-like structure, with an apparent elongation suggesting an inclined orientation relative to the observer. The central region is characterized by a bright, concentrated bulge, exhibiting a yellowish hue. The disk component appears to be somewhat flocculent, hinting at the presence of spiral arms or irregular structures, but these features are not sharply defined. The overall color gradient transitions from the yellowish center to a bluer periphery, potentially indicative of ongoing star formation in the outer regions. There is no obvious evidence of major mergers or strong tidal disturbances, although the subtle irregularities in the disk might suggest minor gravitational interactions.
