The galaxy presents as a flattened, elliptical-like system, viewed at a near edge-on angle. The central bulge exhibits a concentrated, bright yellow-orange hue, suggesting a dominant population of older stars. Extending outward from the bulge, a fainter, relatively smooth disk-like structure can be seen. This disk appears bluer in some portions than the core. No distinct spiral arm structure or prominent dust lanes are apparent in this image. The light distribution suggests a relatively high degree of central concentration. The overall structure is symmetrical and lacks any obvious signs of significant tidal disturbances or interactions with neighboring galaxies.
