The galaxy appears as a somewhat rounded, elliptical-like structure with a concentrated central bulge. It exhibits a smooth texture without prominent spiral arms or significant dust lanes visible in this image. The galaxy presents a yellow-orange hue, possibly indicating a population of older stars and a relatively low star formation rate. There may be a very faint disk but it is hard to discern. There does not appear to be any signs of galactic merging or major disturbance, however there are some small hints that there may have been a minor disturbance in the galaxy's past.