The galaxy presents a relatively smooth, elliptical morphology. It appears concentrated, with a bright, yellowish core that likely indicates an older stellar population. The radial light profile suggests a gradual decrease in surface brightness from the center outwards. There is no clear evidence of prominent spiral arms, bars, or significant dust lanes, indicating that this is likely an early-type galaxy. The color gradient subtly transitions from yellow at the center to slightly redder hues in the outer regions. There is no clear indication of any ongoing major mergers or tidal disturbances in the image, with only slight suggestions of minor asymmetry in the outer halo.
