The galaxy presents as a somewhat elliptical, disk-like structure. The central bulge appears bright and concentrated, exhibiting a yellowish-white hue, suggestive of an older stellar population. The surrounding disk shows a bluer coloration, possibly indicative of ongoing star formation. There may be hints of faint spiral arm structures, but this is not definitive from the image. The galaxy's periphery seems relatively smooth and ill-defined, with no obvious signs of significant tidal disturbances or major merger activity. Overall, the galaxy appears to be a relatively massive system, with evidence of both old and young stellar populations.
