The galaxy appears as a diffuse, yellowish object. It exhibits an irregular morphology, with a noticeable clumpy structure. Several distinct, bright regions are visible within the galaxy's overall form, suggesting localized areas of intense star formation or the presence of distinct galactic substructures. The overall shape tends towards rounded, although deviations indicate it is not perfectly elliptical. There may be signs of tidal interactions or ongoing mergers, implied by the disturbed and asymmetric distribution of the light. The light distribution is dominated by redder bands. This implies a higher population of older, redder stars and/or a significant amount of dust obscuring any blue light from younger stars.
