The galaxy presents as a compact, elliptical-like structure with a smooth, largely featureless appearance. The central region exhibits a high concentration of light, appearing bright and yellowish-gold in color, possibly indicative of an older stellar population. The light gradually fades in intensity as we move outwards from the core. There is very little evidence of distinct spiral arms or prominent dust lanes. The overall shape approximates circular symmetry, with minimal elongation or asymmetry. Subtle color variations suggest the presence of differing stellar populations or minor star formation activity, although this is not immediately obvious. The object's appearance suggests it is a relatively massive system, and probably with a small amount of current star formation.
