The galaxy appears to be a single, relatively luminous object with a somewhat diffuse morphology. Its shape is neither perfectly elliptical nor a clear spiral. The color profile is complex, exhibiting a central region with a concentrated reddish hue, surrounded by a broader, less intense area with a greenish tint. There is evidence for ongoing star formation, possibly at a rate of a few solar masses per year. The galaxy may be undergoing a minor interaction with another galaxy, as there is a small, nearby galaxy in the lower part of the image. There may be some mild disturbance in the outer regions of the main galaxy.
