The galaxy presents as a moderately bright, somewhat elongated structure. The central region is characterized by high luminosity, appearing nearly white, suggesting a concentration of stars and potentially an active galactic nucleus. This core is surrounded by a less intense but broader halo of light, which displays a distinct blue hue. The blueness indicates a relatively younger stellar population with ongoing star formation. On one side of the core, there is a slight extension of greenish light, while on the opposite side, there is a slight extension of bluish light, possibly indicating recent star formation. 

The overall morphology appears relatively smooth, although with some subtle irregularities, and indications of past or ongoing interactions or minor disturbances. The slight asymmetry in the outer regions could be suggestive of tidal interactions.
