The galaxy presents as a disk-shaped system, observed at a moderate inclination relative to our line of sight. The central bulge appears prominent and exhibits a yellowish-white color, indicative of an older stellar population. The disk component displays a bluer hue, suggesting ongoing star formation, though this is more subtle and less extensive. The galaxy appears to have a relatively smooth morphology, with only slight disturbances visible in the disk. There is no strong evidence of a major merger event. Overall, the galaxy seems to be a relatively undisturbed disk galaxy.