The galaxy presents as a somewhat rounded, extended object. The central region displays a concentrated, bright core with a yellowish-orange hue, suggesting an older stellar population. Progressing outwards from the core, there appears to be a diffuse and less structured disk. The colors shift toward greenish-yellow, potentially indicating the presence of younger stars and some ongoing star formation, although the overall star formation activity seems relatively subdued. Irregularities are visible within the disk, possibly minor disturbances or early signs of a merger. A faint, larger structure envelopes the inner parts.