The galaxy presents as a relatively compact object with a generally smooth morphology. There is a slight disk structure visible, but overall the light is fairly uniform, with the object appearing mostly round. The color profile suggests a galaxy containing an older stellar population, as the redder wavelengths are dominant. There may be some on-going star formation occurring, given the hints of bluer light, although the rate appears relatively low. There is no strong evidence of a major ongoing merger, although subtle disturbances or minor interactions cannot be ruled out.
