The galaxy appears to be a relatively small, fairly smooth system with a hint of disk-like morphology. It exhibits a central bulge that transitions smoothly into the outer regions. There's a slight elongation to its shape, deviating from a perfect circle. The galaxy displays a faint blue hue, suggesting the presence of some young stars, although star formation appears generally subdued. No significant spiral arm structures or dust lanes are discernible. There is no apparent interaction or merging activity with neighboring galaxies.
