The galaxy presents as a slightly elongated, disk-like structure. A central bulge is visible, exhibiting a yellowish-orange hue, suggesting an older stellar population. The disk component shows a bluer color profile, indicating the presence of younger stars and possibly ongoing star formation. The overall smoothness of the light distribution suggests a relatively relaxed morphology with minimal signs of recent major mergers or tidal disturbances. Subtle irregularities may be present, hinting at minor gravitational interactions. The galaxy's apparent size is small, and its low surface brightness makes it a challenge to resolve fine details.
