The galaxy presents an elliptical morphology, with a smooth, largely featureless appearance. Its color profile indicates a dominant population of older stars, exhibiting a redder hue in the outer regions. There is some indication of recent star formation, evidenced by the blue light emanating from the central region. No significant spiral arm structure or dust lanes are discernible. The galaxy's roundness suggests it has undergone minimal disturbances due to interactions with other galaxies, but there is a slight disturbance visible. The galaxy's size is moderate, appearing neither overly large nor compact within the image frame.
