This galaxy appears to be a relatively smooth, elliptical galaxy. Its central region presents a concentrated, bright core, with a gradual decrease in luminosity extending outward. The galaxy appears somewhat elongated, with a ratio of the major to minor axis suggesting it is not perfectly spherical. There is a slight color gradient, with a subtle shift toward redder hues in the central region and bluer hues in the outer regions. The lack of distinct spiral arms or dust lanes suggests that this galaxy has little active star formation, with most stars in this galaxy being older. There is no evidence of major disturbances or merging events, as the overall morphology seems undisturbed and well-defined. There may be some indication of a minor disturbance, such as a slight irregularity in the outer regions of the galaxy, but this would need further investigation to confirm. 