The galaxy appears to be a relatively small, potentially disk-shaped system observed at an oblique angle. Its core region exhibits a high degree of luminosity and what appears to be concentrated stellar density, indicated by its bright, nearly uniform hue. There is a visible extension of the central region suggestive of a disk structure. Evident irregularities in the outer regions suggest the presence of galactic features like spiral arms or tidal tails. The overall morphology suggests some form of gravitational disturbance or interaction, with minor asymmetries and possible merger indicators.
