The galaxy presents an elliptical morphology, appearing relatively smooth in structure without prominent spiral arms or a central bar. The light profile appears to decrease smoothly from the center outwards, indicating a high degree of central concentration. A slight elongation is discernible, with a flattening ratio suggesting a moderate ellipticity. The galaxy displays a color gradient, transitioning from a bluer hue at the center to a redder hue in the outer regions. The blue central color possibly implies ongoing or recent star formation in the core, while the redder outskirts likely indicate a population of older, cooler stars. The overall luminosity suggests a relatively moderate size. There is no evidence of significant tidal disturbances or ongoing major mergers. Overall, this galaxy appears to be a relatively undisturbed elliptical system experiencing some low levels of central star formation.
