The galaxy presents as a single, somewhat diffuse object with a moderate size. It exhibits an elliptical morphology, appearing more elongated than perfectly circular, but not significantly cigar-shaped. The galaxy shows an uneven light distribution. There appears to be a brighter, more concentrated central region suggesting a higher density of stars in the core. There are no apparent spiral arm structures or dust lanes visible in this image. There appears to be some merging happening, whether a minor or major disturbance, it cannot be said definitely but there are two distinct parts in the image that indicates that there is potentially an ongoing merging process.
