The galaxy presents a generally smooth, elliptical morphology. It appears largely spheroidal, with a high degree of central concentration, though the resolution limits detailed analysis of internal structure. The color profile suggests a relatively evolved stellar population, trending towards redder wavelengths, indicative of older stars. There is little evidence of active star formation or significant dust lanes. The galaxy does not appear to be undergoing any major mergers, though minor disturbances cannot be ruled out given the limitations of the image quality. It has an estimated size of approximately 7 kiloparsecs in radius.
