The galaxy presents as a fairly smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing largely round in projection. The color profile suggests a dominant older stellar population, indicated by the yellowish-red hue of the galaxy's core. There's some evidence of a subtle blueish component in the outer regions. No strong spiral arm structure or significant dust lanes are apparent. Overall, the galaxy appears relatively undisturbed, showing minimal signs of recent merger activity or tidal interactions.
