The galaxy presents as a moderately inclined spiral, possibly of late-type morphology. The central bulge appears relatively small, and not especially bright, with the majority of the light appearing to originate in the disk. The disk exhibits a notable asymmetry, with a slight warping visible. There appear to be loosely wound spiral arms. There is a slight suggestion of dust lanes in the disk. There may be a bar feature present within the galaxy, but it is not especially distinct. The overall color profile is relatively red, indicating a possible lack of ongoing active star formation. The outskirts of the galaxy appear fairly diffuse. The galaxy does not appear to be undergoing any major interaction.
