The galaxy presents a morphology that is neither strictly elliptical nor a well-defined spiral. The central region exhibits a bright, concentrated core, suggesting a significant stellar population. Extending outwards from this core, a diffuse disk-like structure is apparent, hinting at the presence of spiral arms, albeit somewhat obscured or disrupted.  The galaxy's overall shape is moderately elongated. There appears to be a slight asymmetry in the distribution of light, potentially indicating a past interaction or merger event. One side exhibits a subtle extension or tail-like feature with a reddish color. The blue hue of the central region suggests active star formation.
