The galaxy presents as a complex system, exhibiting characteristics of both a smooth morphology and distinct features, potentially indicative of a disk. There is evidence of ongoing interaction or merging activity. 

The primary component appears somewhat elliptical, displaying a concentration of older stars that manifest as a yellow to red color. This component is connected to a region exhibiting a bluer hue, suggestive of younger, hotter stars and ongoing star formation. This bluer region is less structured, appearing more diffuse and amorphous. 

Distinct disturbances are observable within the galaxy's structure, perhaps arising from a minor merger event. A tidal tail cannot be ruled out based on the overall morphology. The galaxy's overall shape is irregular, and the distribution of light is uneven.
