The galaxy presents as a somewhat flattened, elongated structure. The central region exhibits a brighter, more diffuse luminosity, suggesting a concentrated stellar population or active galactic nucleus. Moving outward from the center, the light becomes less intense with a more granular texture to it. The galaxy appears to have some distortions in its morphology, most notably a slightly elongated shape, possibly indicative of gravitational interactions or a recent merger event. There are also some irregularities within the structure, with an uneven distribution of light and some possible tidal features or disrupted arms. Overall, this galaxy shows characteristics of a system undergoing some form of dynamic interaction or internal disturbance. The bluer color in the center relative to the outer regions suggests some active star formation is present.