The galaxy exhibits a generally elliptical morphology, appearing quite smooth and rounded in shape with no immediately obvious spiral arm structure or significant disk component. It displays a central concentration of luminosity which gradually diminishes towards the outer regions. The core appears to be a yellowish hue, suggestive of an older stellar population. A faint, bluer halo surrounds the galaxy, possibly indicating the presence of some younger, star-forming regions, albeit at a relatively low rate. There is no clear evidence of any ongoing major merger events or significant tidal disturbances, but a minor asymmetry cannot be ruled out.
