The galaxy presents as a generally smooth, elliptical-like structure, with a high degree of central concentration. Its shape is very close to round. There is an apparent extension of light to the galaxy's right-hand side. There are no obvious spiral arms or significant dust lanes visible. The color is mostly white-ish blue, indicating a population of stars with a substantial hot, young component, with some redder color in the halo, which could indicate an older stellar population. There is no visual evidence of a major ongoing merger or tidal disruption, though there seems to be minor disturbances.
