The galaxy appears to be a relatively bright, early-type spiral or lenticular system, with a high degree of central concentration. The central bulge is prominent and appears spheroidal, exhibiting a smooth, featureless appearance. The disk component is visible but less pronounced, with a relatively faint, diffuse structure that fades into the background sky. There is a subtle dust lane, appearing as a slight darkening, that obscures the light from the bulge in the disk, perhaps indicating the presence of a dusty galactic plane, viewed nearly edge-on. The overall color is yellowish-red, indicative of an older stellar population. No prominent star-forming regions or spiral arms are clearly discernible. The galaxy exhibits a flattened shape, suggesting a rotating system.