The galaxy presents a largely smooth morphology, exhibiting a central, somewhat concentrated luminosity. The overall shape appears neither perfectly circular nor highly elongated, displaying an intermediate ellipticity. Faint indications of possible faint outer structures are present, though the image resolution limits a definitive assessment. Color gradients across the galaxy suggest a potentially varied stellar population, with a slightly redder core transitioning to marginally bluer outer regions. No prominent dust lanes or spiral arm structures are readily discernible in this view. Further spectroscopic and high-resolution imaging would be beneficial to clarify the precise morphological classification and internal dynamics.
