The galaxy appears to be a relatively smooth, disk-shaped system seen at an oblique angle. There is a central bulge region that seems well-defined and relatively bright, indicating a concentration of older stars. The overall color profile suggests a population of stars that are likely intermediate in age and/or contain ongoing star formation. The disk component is subtly mottled, possibly due to some internal structure or density variations. The disk extends noticeably beyond the bulge, indicating a spiral structure may be present though not easily distinguished. No obvious signs of major interactions or mergers can be detected.
