This galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a primarily spheroidal morphology. The light distribution suggests a high degree of central concentration with a gradual decline in luminosity moving outward. The core region appears to be yellowish, indicative of an older stellar population dominated by evolved stars. There is some evidence of a slightly bluer halo surrounding the core, potentially indicating the presence of a younger, albeit less prominent, stellar population in the outer regions. There is no apparent spiral arm structure, bar, or significant dust lane obscuration visible within this galaxy. The overall form appears relatively undisturbed, suggesting it is not currently undergoing a major merger event. There may be a slight tidal disturbance, but the morphology is largely undisturbed.
