The galaxy presents as a relatively smooth, centrally concentrated object with a hint of elongation but lacking a pronounced disk structure. The light distribution appears fairly uniform across the galaxy, suggesting an older stellar population. The galaxy appears elliptical in shape, trending towards a more spheroidal morphology. There is a faint suggestion of some irregularity in the outer regions of the galaxy, such as some minor disturbance, but no clear signs of ongoing major mergers or significant tidal interactions are evident. The blueish hue indicates the possibility of some recent star formation. The galaxy has no central bulge.
