The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light distribution. The core appears bright and yellowish, suggesting a population of older stars. There is a slight elongation to the galaxy's overall shape; it is rounded, though not perfectly circular. No distinct spiral arms or bar structures are visible. There are no obvious signs of ongoing major mergers or significant tidal disturbances. Faint blue hues are present in the outer regions, potentially indicating some low level of recent star formation at the outer edges. The galaxy appears to be relatively isolated in this field of view.
