The galaxy appears to be a single, relatively smooth object, likely an elliptical galaxy given its morphology. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the edges, indicating a high degree of central concentration. There is very little evidence of spiral arms or a disk structure; the galaxy is primarily spheroidal. The color appears slightly redder, implying an older stellar population with relatively little ongoing star formation. There are no prominent dust lanes or regions of active star formation visible within this galaxy. There is no signs of tidal disturbances. This galaxy appears to be relatively isolated and undisturbed.
