The galaxy presents as a barred spiral, exhibiting a prominent central bar structure. The spiral arms appear tightly wound, emanating from the ends of the bar and tracing a relatively smooth, continuous path outward. Two dominant spiral arms are discernible. The galaxy appears moderately inclined, with the disk displaying a slightly elongated shape. A central bulge is present, though its relative size appears moderate. The overall color of the galaxy suggests a mix of stellar populations, with the central regions displaying a whiter hue, possibly indicating older stars, while the outer arms exhibit a slightly bluer tint, potentially indicative of ongoing star formation. There is no apparent evidence of major mergers or significant tidal disturbances in this image, suggesting a relatively isolated and unperturbed system.
