The galaxy presents as a somewhat elliptical structure, exhibiting a dominant central bulge. The bulge appears to be primarily composed of older stellar populations, judging by its yellowish hue. This contrasts with the disk, which displays bluer colors indicative of younger, hotter stars and ongoing star formation. The disk also has regions of redder emission. Overall, the galaxy seems to be relatively smooth in appearance, lacking prominent spiral arms. There is a slight distortion in the morphology, which may be the result of a minor gravitational interaction or internal dynamics. The galaxy is of moderate size.
