The galaxy appears as a single, concentrated object with a fairly smooth and centrally concentrated light distribution. It exhibits a predominantly elliptical morphology, appearing almost perfectly round from our viewing angle. There is no evident disk structure or spiral arm features. The galaxy's core region displays a yellowish hue, suggesting an older stellar population. There are hints of cooler stars in the surrounding area. No signs of significant tidal disturbances, mergers, or interacting companions are immediately apparent. This galaxy appears to be an elliptical galaxy with a high degree of central concentration and a mature stellar population.
