The galaxy presents a generally smooth morphology. The central region displays a high concentration of light, appearing yellow-white. A region extending slightly to the right is redder in color than the main body of the galaxy. This may indicate a region of ongoing star formation, dust obscuration, or an older stellar population. There are hints of very slight disturbances in the overall form, with minor asymmetries, but overall it seems to be a relatively settled structure. It does not appear to be undergoing a major merger, though could be experiencing some minor gravitational interaction. The galaxy exhibits moderate intrinsic luminosity. Its redshift suggests that it is at an intermediate cosmological distance.
