The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated luminosity profile, with a bright, nearly spherical core that gradually fades into the outer regions. There is little evidence of spiral arm structure or significant dust lanes. The galaxy presents a yellowish-white hue, suggestive of an older stellar population and reduced ongoing star formation. There may be a very faint, diffuse halo surrounding the main body of the galaxy, although its visibility is limited. Overall, the galaxy's morphology suggests it is a passively evolving system, nearing the red sequence.
