The galaxy appears to be a relatively compact object with a disturbed morphology. The light distribution is not smooth, indicating possible recent interactions or internal processes. It shows evidence of both smooth and more featured components, exhibiting a complex structure. The color profile suggests a mix of stellar populations, with a bluer central region that might indicate ongoing star formation, contrasted by a redder component indicating older stars, possibly in a bulge or halo. Indications of some tidal disturbances or minor merging are visible.
