The galaxy appears to be a spiral galaxy, though the spiral arms are not distinctly defined. It displays a prominent central bulge which is bright and appears relatively smooth, suggesting a high concentration of older stars. The disk is visible, although the inclination angle makes it appear elongated or cigar-shaped. The light distribution suggests a relatively smooth profile, potentially indicating a lack of significant ongoing star formation within the disk. There's a slight asymmetry or possible minor disturbance in the outer regions, but no obvious signs of a major ongoing merger event. The estimated size indicates that the galaxy is a fairly typical galaxy in the local universe. The overall color is indicative of older stellar populations, implying a relatively low star formation rate for a galaxy of its size.
