The galaxy presents a generally smooth, elliptical morphology. Its central region exhibits a bright, concentrated core, suggesting a high stellar density, possibly indicative of an aging stellar population. The light gradually decreases moving outwards from the core. The body of the galaxy appears largely featureless, lacking any obvious spiral arm structures or prominent dust lanes. There may be very faint traces of a disk structure, though they are not particularly clear. There is no obvious signs of galactic merger or major disturbance. The overall shape is approximately round.
