The galaxy presents a defined, though not perfectly circular, disk structure, viewed approximately face-on. Spiral arms are visible but not particularly well-defined; they appear tightly wound around a central bulge. The bulge is moderately sized, contributing significantly to the overall luminosity of the galaxy.

The color profile suggests the presence of both older stellar populations, contributing to the reddish hues in the bulge, and younger, bluer stars populating the spiral arms. Some dust lanes might exist within the spiral arms, obscuring some of the starlight and creating an uneven texture. There does not appear to be any strong evidence of a bar structure. The galaxy does not show significant morphological distortions indicative of major merger activity. Faint disturbances or minor mergers may not be discounted.
