The galaxy presents as a centrally concentrated object with a relatively smooth overall appearance. Its shape is generally elliptical, tending towards round, with a slight elongation. The core exhibits a bright, yellowish hue. Fainter, greenish tinges are observable in the surrounding regions of the galaxy, perhaps indicating areas of lower stellar density, or regions with younger stars. There is no clear evidence of spiral arm structure or a prominent disk component. No significant signs of tidal disturbances, major mergers, or strong gravitational interactions are visible. The galaxy seems to be a relatively isolated system in a fairly advanced stage of morphological evolution.
