The galaxy presents as a flattened, disk-shaped structure, oriented nearly edge-on relative to our line of sight. The central bulge region is relatively bright and appears yellowish-white, possibly indicative of an older stellar population. Fainter light extends outwards from the central bulge in a flattened distribution, which suggests a galactic disk. The light gradually fades away from the central bulge region.

The disk structure shows some evidence of internal structure. There appear to be slight irregularities. There does not appear to be any spiral arm structure. Based on the estimated mass, the galaxy is relatively massive. The inferred star formation rate indicates that star formation activity is relatively subdued. Overall, this appears to be a relatively quiet galaxy exhibiting low levels of merger activity.
