The galaxy presents a predominantly smooth morphology. The structure appears elliptical with a notable lack of distinct spiral arms or features. The shape is not perfectly round; rather, it exhibits a slightly elongated, cigar-like form. There is no clear indication of ongoing major merger activity. The galaxy displays a smooth light profile, concentrated towards the center. It has a moderate size and luminosity. It shows a dimness in blue light, trending to a brighter red. This indicates there is a population of older stars and little ongoing star formation, confirmed by the fact that any disk components are not very luminous.
