The galaxy presents as a roughly elliptical, centralized object. Its core exhibits a bright, concentrated emission, appearing yellowish-white in color, suggesting a population of older stars. The light diminishes gradually outwards from the center. A fainter, distinct region is visible near the primary body, possibly a satellite galaxy or a region of enhanced star formation. This region is distinctly bluer in color. The overall morphology suggests a relatively smooth structure, though minor disturbances or tidal features cannot be completely ruled out at this resolution. The shape is generally round. Evidence suggests that the galaxy may be interacting or merging with another smaller galaxy.
