The galaxy appears as a relatively smooth, elliptical structure, characterized by a concentrated central bulge. There is minimal evidence of distinct spiral arms or prominent dust lanes. The overall color is a yellowish-orange hue, suggesting a population of older stars. The galaxy displays an intermediate ellipticity, appearing neither perfectly spherical nor highly elongated. There are no obvious signs of major mergers or significant tidal disturbances affecting its morphology, though there are some minor indications of potential faint disturbance.
