The galaxy appears as a concentrated central region with a predominantly smooth morphology. The overall color leans towards redder hues, suggesting a population of older stars or significant dust obscuration. There is little to no evidence of spiral arm structure or a prominent disk. The shape is generally round. No major disturbances from mergers are evident, though minor interactions cannot be entirely ruled out. The galaxy exhibits a relatively high rate of star formation for its stellar mass. The overall impression is of a relatively compact and quiescent system.
