The galaxy presents a somewhat amorphous, elongated form. Its overall color profile suggests a mix of stellar populations, with a central, brighter region exhibiting a whiter hue, indicating a possibly older stellar population or dust obscuration. Extending outward from this central area are fainter, bluer tendrils or arm-like structures, particularly toward one end of the galaxy. These regions indicate areas of ongoing star formation and a younger population of stars.

The light distribution is uneven, with a prominent, condensed core and more diffuse outer regions. There appear to be some subtle irregularities and potential disturbances in the outer edges of the galaxy, suggesting potential interactions or past mergers. No strong spiral arm structure is evident; instead, the light is more uniformly distributed across the disk. The galaxy appears relatively undisturbed, lacking strong tidal tails or prominent signs of active merging. The galaxy is relatively compact, estimated at approximately 5-6 kiloparsecs in radius.
