The galaxy presents as a centrally concentrated object, exhibiting a near-spherical morphology. The light distribution is dominated by a smooth, centrally bright component, with a falloff in luminosity toward the outer regions. There is a hint of color variation, with the central region appearing more yellow, possibly indicating an older stellar population. No spiral arms or obvious disk structures are discernible. There are no apparent signs of significant tidal disturbances, major mergers, or interacting companions. Faint features around the galaxy indicate the slight possibility of minor disturbances.
