The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology. The central region is significantly brighter, suggesting a bulge component. A faint, diffuse halo or disk-like structure extends outward from the central bulge, though its features are not well-defined. There may be a slight flattening, making the morphology slightly elliptical. There does not appear to be any significant evidence of spiral arm structure or prominent dust lanes. There are no obvious signs of recent major merger activity. The color indices suggest that the galaxy is comprised of older stellar populations, with a relatively low ongoing rate of star formation. The galaxy shows a redder hue in the central region and a more blueish hue in the outer regions, suggesting older stars in the center and younger stars in the disk.
