The galaxy appears as a centrally concentrated object with a generally smooth, elliptical morphology. Its color is slightly reddish, indicating a population of older stars and a relatively low current star formation rate. The galaxy exhibits a subtle radial gradient in surface brightness, with a brighter core that gradually fades into the outer regions. There is no clear evidence of spiral arm structure or a prominent dust lane. A small disturbance can be seen, such as a minor asymmetry in the outer halo which may be indicative of a past or ongoing minor merger event. The absence of distinct features suggests that the galaxy is likely an evolved system that has largely exhausted its supply of gas.
