The galaxy presents a primarily smooth morphology, exhibiting a centralized concentration of light. The galaxy’s shape appears somewhat elongated, but not excessively so. The object appears relatively undisturbed, showing no signs of a major merger, although there may be some minor distortion of the galaxy. The color profile suggests a mix of stellar populations, with a central region appearing more yellowish, indicative of older, redder stars, and outer regions exhibiting a bluer hue, suggesting the presence of younger, hotter stars. Overall, the galaxy appears to be a disk galaxy with a moderately high mass, undergoing a moderate amount of star formation.
