The galaxy exhibits a central, bright core region that appears roughly elliptical in shape. A diffuse, extended halo surrounds the core, displaying a gradient in color. The core is predominantly blue-white, suggesting a significant population of young, hot stars. The outer halo transitions to a greenish-blue hue and then a dark purplish tone, which may indicate the presence of older stellar populations and dust.

The overall morphology appears somewhat irregular, with subtle disturbances or asymmetries visible in the halo's structure. There is a hint of a possible tidal tail or minor disruption, but a significant portion of the galaxy has a somewhat smooth appearance, particularly in the central region. There is some evidence of a more complex structure in the immediate vicinity of the core, suggesting ongoing star formation. However, the object seems relatively intact, with no obvious signs of complete disruption. The image suggests the possibility of a recent or ongoing interaction with a smaller object, contributing to the observed irregularities.
