The galaxy appears as a somewhat elongated, cigar-shaped structure with a prominent central bulge. The core region exhibits a bright, concentrated luminosity, suggesting a high density of stars or potentially an active galactic nucleus. The overall color gradient indicates a range of stellar populations, with the core trending towards redder hues and the outer regions displaying a bluer tint. This could imply a concentration of older stars in the central bulge and ongoing star formation in the surrounding disk. There is some evidence of a faint, asymmetrical disk structure, suggesting a possible disturbance or interaction with another galaxy. The smooth appearance suggests a relatively evolved system, although the bluer color in the outer regions indicates some recent or ongoing star formation. There is no clear evidence of strong spiral arms, and the overall morphology suggests it is transitioning towards a more elliptical shape.
