The galaxy appears as a somewhat elliptical, though slightly irregular, extended source. There is a bright, concentrated central bulge that dominates the overall luminosity. The light from the bulge is whitish-yellow, suggesting a population of older stars.

Surrounding the bulge, a fainter, more diffuse disk is visible. The disk component shows subtle hints of bluer light, suggestive of more recent or ongoing star formation. Some irregularities in the disk's structure hint at possible past or ongoing interactions.

The galaxy exhibits a color gradient, transitioning from bluer regions in the outer disk to a more yellow/red color toward the central bulge. Overall, the galaxy is not perfectly smooth and has some visible features in the disk.
