The galaxy presents as a slightly tilted, disk-shaped structure. Its central region exhibits a concentrated, bright luminosity, indicative of a significant stellar population and possibly an active galactic nucleus, which fades into bluer hues, suggestive of younger stars and ongoing star formation.

The galaxy's disk appears relatively smooth, lacking the distinct spiral arm structure often seen in spiral galaxies. The light is elongated, suggesting a bar-like structure within the galactic center. There is a slight hint of disturbance in the outer regions of the galaxy, possibly indicating minor gravitational interactions or past mergers. Overall, the galaxy appears to be a galaxy in the early stages of its development.
