The galaxy appears to be a relatively smooth, elliptical type galaxy at a considerable distance. It exhibits a centrally concentrated, bright core that gradually fades outwards. The overall shape is mostly smooth, with minimal evidence of spiral arm structures or irregular features. The galaxy appears to have a slight ellipticity, deviating somewhat from a perfect circle. The color profile suggests a dominant population of older stars, with a yellowish hue in the central region. There may be some faint, bluer regions surrounding the core. These areas may indicate younger star formation, although the overall smoothness suggests it is not dominant. There are no apparent signs of recent major merger activity or tidal disturbances. Based on the observed morphology and color, the galaxy could be an early-type system approaching quiescence.
