The galaxy appears as a concentrated, elliptical-like structure, exhibiting a generally smooth morphology. There is some indication of a possible merging event or minor disturbance within the system, shown by an asymmetric shape in the bottom left. Overall, the distribution of light is centrally concentrated, diminishing gradually outwards from the core. The primary color gradient is consistent with a population of older stars and dust obscuration. There is some evidence of ongoing or recent star formation, evidenced by the blue light present within the core. The angular size of the galaxy suggests that this is a fairly distant galaxy, observed at a redshift of approximately 0.385536.
