The galaxy presents as a diffuse, irregularly shaped object with an apparent radial size of approximately 8 arcseconds. Its overall color profile suggests a dominant population of older stars, showing a gradient from a bluer hue toward what appears to be a disk region and trending toward redder tones in the outer regions.

The central area is characterized by a relatively smooth and featureless appearance, while towards the periphery, there's evidence of subtle structural features. Patchy regions of bluer light suggest areas of ongoing or recent star formation. There is a possible disruption or irregularity on one side, potentially indicative of a minor gravitational interaction or internal dynamic process.
