The galaxy presents as a spiral type, likely at a relatively early stage of development based on observed star formation. Its apparent size indicates a moderately sized galaxy, with a discernible central bulge and spiral arms that are beginning to emerge.

The central bulge exhibits a smooth, concentrated luminosity profile, suggesting an older stellar population. The spiral arms are less defined, displaying a mottled appearance with pockets of active star formation. These regions are characterized by a bluer hue compared to the more yellow-red color of the central bulge, indicating a younger, hotter stellar population.

There appears to be a degree of disturbance in the spiral structure, possibly indicative of a minor gravitational interaction with a smaller companion galaxy or past merger event. One arm appears slightly distorted, suggestive of tidal forces acting on the galactic disk. There is no clear indication of a prominent bar structure.
