The galaxy presents as a relatively smooth, elliptical structure with a noticeable central bulge. The galaxy exhibits a color gradient, transitioning from a yellowish-orange core to a bluer halo or outer region. This suggests a radial variation in stellar populations, with older, redder stars concentrated in the center and younger, bluer stars more prevalent in the outer regions. There are no clear spiral arms or distinct dust lanes visible. The overall shape appears to be somewhat elongated, but not highly flattened. No significant signs of tidal interactions or major mergers are immediately apparent in the image, though there is some slight asymmetry in its outer regions. The galaxy's color indicates moderate levels of on-going star formation.
