The galaxy appears as a relatively compact object with an ellipsoidal morphology. Its spatial extent is small within the image frame.

The color profile suggests a complex stellar population. A central, bright, and slightly elongated region dominates the galaxy's light. This core exhibits a bluer hue compared to the outer regions, possibly indicating recent star formation activity within the nuclear region.

There is evidence of a disk-like feature, but it appears faint and less distinct. The outer regions of the galaxy display a more diffuse and irregular structure. I observe at least one possible tidal stream feature or minor disturbance in the surrounding halo region.

The galaxy does not present a classical spiral structure, and might be undergoing a minor merger event, or recent dynamical interaction.
