The galaxy presents as a relatively smooth, disk-like structure viewed at an oblique angle. The central region exhibits a concentrated luminosity, appearing significantly brighter and yellower than the outer regions of the disk. The light distribution suggests an older stellar population dominating the core.

Moving outward from the core, the disk becomes less luminous and exhibits a bluer color. There are subtle hints of spiral arm structure or irregularities in the disk, though they are not prominently defined. Faint color variations within the disk hint at regions of potentially differing stellar populations and ongoing, albeit low, star formation.

Overall, the galaxy appears to be a relatively massive system with a dominant bulge. Evidence points toward it being an intermediate stage between a spiral and elliptical morphology, lacking strong spiral arm definition and possessing a relatively smooth overall structure. It does not appear to be currently undergoing any major merging events, but subtle distortions suggest a possible minor disturbance in the past.
