The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is a noticeable color gradient, trending from a yellowish core to a redder halo region suggesting aging stellar populations. The overall morphology appears undisturbed, without any prominent tidal features or signs of ongoing major mergers. It is fairly symmetrical, with a high degree of central concentration. There are no obvious spiral arm structures. The galaxy appears to be a dominant, isolated object.
