The galaxy presents a slightly elongated, disc-like morphology. It appears relatively smooth, with a high degree of central concentration of light. There is some suggestion of a faint spiral structure, although it is not particularly well-defined. The color gradient suggests a slightly bluer core region with redder outer regions. The galaxy does not seem to be undergoing any major mergers or tidal disturbances, but there is a very slight asymmetry in the spiral arm structure that could indicate a minor interaction with a smaller object. Overall, the galaxy appears as a fairly typical spiral galaxy at some distance.