The galaxy presents as an elongated, roughly elliptical structure. Its core region exhibits a concentrated, yellowish-white luminosity, suggesting an older stellar population. The overall form indicates a spheroidal morphology, with a smooth, featureless appearance that is consistent with an early-type galaxy, such as an elliptical or lenticular. There is a subtle hint of a disk-like structure surrounding the central bulge, which is oriented at an angle relative to our line of sight. The outer regions of the galaxy appear somewhat fainter, and show areas of bluish light, possibly indicating regions of younger stellar populations. There is no obvious evidence of spiral arms or prominent dust lanes. The overall appearance suggests a mature, relatively quiescent system with a relatively low star formation rate.
