The galaxy presents a generally smooth morphology, exhibiting a bright central bulge that dominates the overall structure. There appears to be some irregularity to the right side of the galaxy. The color distribution suggests a higher concentration of older stellar populations in the central region, indicated by the redder hue, while the bluer regions toward the periphery may indicate ongoing star formation. Some distortions are evident in the galaxy's form, possibly suggestive of a minor gravitational interaction, with a small arm or tidal feature. Overall, the galaxy appears to be relatively compact with a roughly elliptical shape.
