The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a largely elliptical morphology, appearing almost perfectly round. There is no obvious indication of significant spiral arm structure or a prominent disk component. There is no sign of ongoing major merger activity, although some minor tidal disturbances cannot be completely ruled out. The galaxy has an intrinsic size of several kiloparsecs and exhibits a moderate redshift, indicating a significant distance. The galaxy appears primarily quiescent, exhibiting relatively low rates of star formation. Based on its color, it appears to be comprised of a population of relatively older stars. 
