The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated light profile with no discernible spiral arms or bar structures. The central region displays a bright, relatively uniform luminosity, suggestive of a significant population of older stars. The galaxy's color is primarily yellow-orange, which may indicate a lack of ongoing star formation, and a dominant population of older, cooler stars. There is no visual evidence of dust lanes or gas clouds associated with active star forming regions. Overall, the galaxy appears as a well-defined, spheroidal structure with a relatively quiescent stellar population.
