The galaxy presents as a system exhibiting both smooth and potentially disturbed characteristics. Its overall form appears somewhat elliptical, but with subtle irregularities suggesting possible interactions.

The color distribution within the galaxy is not uniform. A bluer hue is observed towards one region, possibly indicating a concentration of younger, hotter stars and ongoing star formation. The bluer region does not appear to be resolved into individual stars, indicating that it is a far away system.

The primary structure of the galaxy seems to be experiencing some level of gravitational disturbance. This disturbance could indicate an ongoing or recent merger event with another galaxy or a tidal interaction with a nearby object. Further investigation into the surrounding galactic environment would be necessary to confirm the cause.

The galaxy exhibits a moderate redshift, placing it at a considerable distance.
