The galaxy exhibits a generally smooth morphology, with a discernible, elongated shape. It appears to be elliptical or lenticular, exhibiting a central bulge that gradually fades outwards. The galaxy's light is concentrated towards the core, suggesting an older stellar population, with little evidence of active star formation discernible in the image. There may be some subtle hints of a very faint disk, but it is predominantly bulge dominated. The overall color appears slightly redder. There are no signs of tidal tails or other obvious merger features. The galaxy appears isolated.
