The galaxy presents as a spiral galaxy, observed face-on, with a clearly discernible disk structure. The central bulge appears moderately sized and displays a yellowish hue, suggesting an older stellar population. Faint, tightly wound spiral arms emanate from the bulge, exhibiting patches of bluer light indicative of ongoing star formation. The galaxy is not perfectly symmetrical, with a slight asymmetry noted in the distribution of the spiral arms. There is no strong evidence of a prominent bar structure. The disk appears relatively smooth, with some subtle irregularities likely due to dust lanes or localized star-forming regions. The galaxy displays a somewhat amorphous shape, lacking a clear, well-defined edge. Overall, it presents as a moderately active spiral galaxy with a mix of stellar populations.
