The galaxy presents as a relatively compact object. It exhibits a bright, spheroidal central region, likely indicative of a prominent bulge. A fainter, more diffuse component extends from this core. Subtle color variations are observable, with a hint of bluer tones in the outer regions, potentially indicating younger stellar populations or ongoing star formation, and redder tones in the bulge. This suggests a possible gradient in stellar age across the galaxy's structure. The overall morphology suggests a system that is neither purely elliptical nor a well-defined spiral, but rather a galaxy with both a smooth, spheroid structure and some degree of disk-like feature. There's evidence of a possible interaction or minor disturbance in its shape.
