The galaxy presents as a relatively compact object. Its morphology appears largely smooth, with a central, bright, unresolved core. This core exhibits a distinct blue hue, suggesting a population of hot, young stars, possibly indicative of ongoing star formation within this region.

Surrounding the bright core, there is a diffuse halo of light. This halo is not uniform in color. Faint, reddish-yellow patches are observed extending from the core. These features may represent older stellar populations, dust lanes, or regions of diminished star formation. The overall structure does not obviously suggest a spiral disk, although it is not possible to entirely rule out some disk component. There is some evidence of possible minor disturbance of the galaxys structure.
