The galaxy exhibits a generally smooth morphology with a relatively concentrated core. The central region presents a bright, almost unresolved appearance. There is faint, extended structure visible around the core, suggesting a possible disk or halo component, though this structure is poorly defined and could also be due to artifacts. The galaxy displays a blue hue in the central regions, possibly indicative of recent star formation. Fainter, redder material is visible in the outer regions. There's a possible indication of a slight disturbance in the galaxy's symmetry, potentially suggesting a minor interaction or internal dynamical processes, though the low resolution makes it difficult to ascertain the true nature.
