The galaxy presents as a well-defined, disk-shaped structure viewed nearly edge-on. A prominent central bulge dominates the galaxy's core, exhibiting a concentrated, yellowish hue. This suggests a population of older stars. The disk itself appears relatively smooth, with limited observable dust lanes or spiral arm structures. The lack of significant blue color suggests a low ongoing rate of star formation. Subtle disturbances in the outer disk, such as possible tidal streams, may be present, hinting at potential past interactions with another galaxy. The galaxy is relatively large. Overall, the galaxy morphology suggests an evolved disk galaxy dominated by an older stellar population with minimal current star formation activity and signs of potential past gravitational interactions.
