The galaxy presents as a spiral galaxy with a clear disk structure. Its orientation is face-on relative to our line of sight. Two spiral arms appear dominant and well-defined. There is evidence of active star formation within the spiral arms, with hints of blue-ish regions suggesting the presence of young, hot stars. The central bulge is moderately sized and displays a yellowish-white hue, likely indicating a population of older stars. No significant bar structure is immediately apparent. Overall, the galaxy's morphology suggests it is relatively undisturbed, with no clear signs of ongoing major mergers, though some minor interaction cannot be entirely ruled out.
