The galaxy appears to be a spiral galaxy, observed at an inclined angle, possibly nearing edge-on. A central bulge is visible with a yellowish-orange hue. There is an indication of a disk structure surrounding the bulge, displaying a subtle bluish tint, especially at the outer edges, suggesting the presence of younger stellar populations. The galaxy exhibits a relatively smooth appearance, with no obvious signs of major mergers or significant tidal disturbances. The overall morphology appears to be consistent with a galaxy that has experienced relatively quiescent evolution, with ongoing star formation primarily located in the disk. The central bulge dominates the overall luminosity, hinting at a significant population of older stars.
