The galaxy appears as a centrally concentrated object with a smooth, luminous profile. It has an elliptical morphology, appearing more oblate than prolate. The core exhibits a bright, yellowish hue, suggesting an older stellar population dominating the nuclear region. The light gradually fades as it extends outward from the core. The outer regions display a faint, diffuse glow. There are very subtle hints of structure but it mostly presents as smooth. There is no sign of distinct spiral arms, bars, or dust lanes visible in this image. The lack of blue light suggests a low rate of on-going star formation within the galaxy. There might be slight signs of tidal disturbances. Overall, this galaxy is likely an early-type galaxy, possibly an elliptical or lenticular galaxy, with a well-established, older stellar population.
