The observed galaxy presents as a relatively face-on spiral, exhibiting a defined central bulge region that appears to be moderately sized. The bulge appears to have a yellowish color profile, indicative of an older stellar population. Faint spiral arms are visible, exhibiting a somewhat flocculent morphology, without sharp definition. These arms have a bluer hue, potentially indicating regions of ongoing star formation. The overall structure lacks a strong central bar feature, although a subtle elongation through the bulge might be present. No signs of major mergers or significant tidal disturbances are observed in the primary galactic structure. The disk of the galaxy shows subtle dust lane features, which could be affecting the overall visual appearance, along with some level of patchiness, indicative of heterogeneous stellar distribution throughout the galaxy.
