The galaxy appears to be a single, moderately-sized object with a relatively smooth, diffuse light distribution. The overall shape is somewhat elongated but not highly flattened, trending more towards elliptical than disk-like. A slight asymmetry is noted in the light distribution, where the light appears to be a little more focused on one side of the galaxy and slightly more spread out and diffuse on the other. The core is moderately bright, but there is no clearly defined nucleus. The light diminishes gradually from the core outwards without any obvious spiral arms or other distinct features. There is some suggestion of possible tidal disturbance or a minor merger event hinted at by subtle deviations from a perfectly smooth profile.