The galaxy presents as a relatively compact object. The core region exhibits a high degree of brightness, indicating significant stellar density or active galactic nucleus activity. Moving outward from the core, there is a noticeable decrease in luminosity.

The galaxy displays some disturbed features. A faint extension is visible on one side of the galaxy, suggesting a possible tidal interaction or recent merger event, but the core of the galaxy is relatively undisturbed. The overall morphology appears irregular, lacking the clear spiral arm structure. The color profile of the object is also interesting. There are some colors in the core of the object that are a mix of blue and green. The overall shape is somewhat irregular, and there is some evidence of possible tidal features or asymmetry. Further observations, particularly spectroscopic data, would be beneficial in characterizing the stellar populations and dynamics of this system.
