The galaxy presents as a moderately elongated, cigar-shaped structure with a relatively smooth and diffuse appearance. Its color profile suggests a mixture of stellar populations, with a predominantly yellowish-orange hue indicative of older stars and possibly dust. The central region appears slightly brighter and more concentrated, suggesting a central bulge. Faint blueish tinges are visible at the periphery indicating the presence of younger, hotter stars. Some minor disturbances seem to be present, although the overall structure suggests that the galaxy is not currently undergoing a major merger event. There is no prominent spiral arm structure visible, and its size and shape suggest a galaxy with a substantial mass. Star formation seems to be happening at a slower rate than other active galaxies. 
