The galaxy presents as a moderately bright, compact object. It exhibits a slightly irregular morphology, appearing somewhat elliptical but lacking a well-defined structure. There is a faint halo of diffuse light surrounding the central region, indicating a gradual decrease in luminosity with increasing radial distance.

The color profile reveals a predominantly greenish hue, suggesting ongoing star formation activity. The blue core further implies the presence of young, hot stars. The lack of prominent spiral arms or a central bar suggests the absence of a highly ordered structure, potentially indicative of a recently merged or disturbed system. Faint signs of possible tidal features or minor disturbances exist, which are not obviously symmetric and suggest the possibility of ongoing interactions.
