The galaxy appears to be a spiral type, though the arms are not well-defined, exhibiting a flocculent structure. The central bulge is bright and somewhat concentrated, suggesting an older stellar population. The overall color is a mix of blue and yellow, with hints of redder regions, possibly indicating a combination of ongoing star formation and older stellar populations. There is evidence of minor disturbances in the galaxy's structure, possibly from a past interaction or merger event. The galaxy exhibits an intermediate disk inclination.
