The galaxy appears as a flattened, disk-shaped structure viewed nearly edge-on. A prominent central bulge dominates the luminosity profile, appearing yellowish-white. Fainter, bluer light is visible along the edges of the disk, indicating the presence of a stellar population that may be younger or hotter. The disk exhibits a relatively smooth appearance, suggesting it may be a lenticular or spiral galaxy, with indications of structure within the disk suggesting the presence of spiral arms. There is no strong evidence of a recent major merger or significant tidal disruption, but subtle asymmetries or distortions could point to minor interactions. The galaxy is moderately bright, suggesting a substantial stellar mass. The small angular size of the galaxy, combined with its apparent brightness, implies it may have a moderate luminosity.
