The galaxy presents as a luminous, somewhat elliptical structure with a generally smooth appearance. There is evidence of multiple distinct light concentrations within the galaxy's body, suggesting ongoing or recent merger activity. These concentrations display color variation, with some regions appearing more yellow/orange, potentially indicative of older stellar populations, and other regions showing hints of bluer light, which could be associated with younger, hotter stars forming in the merging event. Overall, the galaxy appears to be undergoing significant dynamical disturbance. The galaxy is of moderate angular size.
