The galaxy presents an elliptical morphology, appearing largely smooth and diffuse in structure. It exhibits a noticeable elongation, transitioning from a more rounded to a slightly cigar-shaped appearance. There are no immediately apparent signs of major disturbances indicative of recent or ongoing major mergers, although there are no signs of spiral arms or a significant disk, indicating that it is most likely an elliptical galaxy. The light distribution suggests a gradual decline in brightness from the central region outwards. The color profile shows a dominant yellowish-red hue, possibly indicative of an older stellar population. The overall appearance suggests a galaxy towards the higher end of the mass scale with a moderate rate of star formation. 
