The galaxy appears to be a spiral type, although the spiral arms are not sharply defined. There is a noticeable central bulge, which exhibits a yellowish hue, suggesting an older stellar population is dominant. The disk surrounding the bulge is relatively smooth with only hints of structure, and a bluish color, implying ongoing star formation, although at a moderate rate. Overall the galaxy appears to be relatively undisturbed, showing no strong evidence of recent major mergers. There might be a hint of a minor interaction or tidal feature. The galaxy has an intermediate roundness.
