The galaxy presents as a disk-shaped structure with a noticeable central bulge. The light distribution suggests a concentration of older stellar populations in the bulge, while the disk exhibits a bluer hue, indicative of ongoing or recent star formation. The disk does not appear to have well-defined spiral arms. There are some morphological disturbances visible, with a minor distortion that could indicate a previous merger or interaction. The galaxy's light is smooth with some asymmetric features.
