The galaxy presents as a relatively smooth, elliptical-like structure. It displays a concentrated central bulge that is yellowish-white in color, indicative of an older stellar population. The outer regions of the galaxy appear less concentrated, with a somewhat elongated shape. The color gradient transitions from yellowish-white in the center to a slightly redder hue in the outer regions, which could be attributed to the presence of dust or a shift in the stellar population. There are no apparent spiral arms or significant dust lanes visible in this image. The overall morphology suggests it is a galaxy with a dominant spheroidal component. It appears undisturbed, with no signs of major mergers or tidal interactions.
