The galaxy presents a largely smooth, centrally concentrated morphology. Its overall shape appears approximately circular. The light is concentrated in a central bulge which seems to make up the bulk of the overall light being emitted by this galaxy. There is a gradient of intensity, with peak intensity at its core and a gradual decrease towards the outer regions. Faint, diffuse material may exist at the edges but there is no definitive presence of spiral arm structures or distinct features visible. It appears as an isolated system, with no clear signs of ongoing or recent major mergers or tidal interactions. There is some slight color variation, but the overall coloration indicates that this galaxy may consist of aging stars, with few or no recent star-forming regions.
