The galaxy presents as a largely spheroidal object with a smooth light distribution, indicative of an elliptical morphology. The central region exhibits a bright, concentrated core. A faint, diffuse halo appears to extend outwards, most notably towards the left side of the image. There is a hint of disturbance in the halo region, although not overtly indicative of a major merger event. The color profile suggests an older stellar population, with a yellowish-red hue dominant throughout the galaxy. Evidence of spiral arms or active star formation regions is not readily apparent. The overall appearance aligns with a relatively evolved galaxy that may be in the process of quiescence.
