The galaxy presents a moderately bright, disk-like morphology. The central bulge appears prominent and exhibits a smooth texture, possibly indicating an older stellar population. A faint, but distinct, spiral arm structure is apparent, with some areas displaying clumpy star formation regions. There are no major signs of ongoing mergers or significant tidal disturbances. Overall the galaxy appears relatively undisturbed. The color profile suggests a diverse stellar population with varying degrees of star formation.
