The galaxy presents as a spiral galaxy with a prominent, moderately sized bulge. The spiral arms are readily visible and appear somewhat tightly wound. The galaxy's disk appears slightly tilted relative to our line of sight. There is no strong evidence of a bar structure bisecting the bulge. The arms display clumpy regions of star formation. The galaxy's color suggests a mix of stellar populations, with the bulge exhibiting a more yellowish hue and the arms displaying more blue colors, indicative of ongoing star formation. There do not appear to be any major mergers or disturbances in the galaxy's overall structure, although the possibility of minor interactions cannot be ruled out. The nucleus is bright.
