The galaxy presents as a singular, moderately bright object with a concentrated central region. It appears to be undergoing a possible interaction or merger, evidenced by a disturbed morphology and the presence of faint, extended features emanating from the main body.

The primary component exhibits a yellow-greenish hue, suggesting a mix of stellar populations, likely dominated by older stars with some ongoing star formation.  The overall shape is somewhat elliptical, though deviations are present due to the observed disturbances. There appear to be several distinct luminous regions around the galaxy, indicating tidal tails or disrupted satellite galaxies merging with the primary galaxy.  These regions vary in color; some appear bluer indicating possibly younger stars. The overall structure appears complex and not well-defined, indicative of a dynamic system possibly in the process of merging.
