The galaxy presents a largely smooth and centralized morphology. The light distribution appears concentrated, with a bright, somewhat indistinct core. Its overall shape is elliptical, appearing mostly round, tending slightly toward a more elongated form. There is little evidence of prominent spiral arms or distinct disk-like features. 

The color profile suggests a primarily older stellar population. The dominant hue is a yellow-orange, indicative of evolved stars and reduced recent star formation. There are subtle hints of bluer regions. These bluer regions are located on the periphery of the galaxy and may point to pockets of younger stars or ongoing star formation, though such activity appears limited.

No strong tidal features, such as plumes or tails, are readily apparent, suggesting that the galaxy has not undergone a major merger event recently. There may be some minor disturbances in its structure, but they are not immediately obvious in this image.
