The galaxy presents a primarily smooth, elliptical morphology. The light distribution is centrally concentrated with a gradual decline in intensity towards the outer regions. No distinct spiral arm structures or prominent dust lanes are apparent. There is a slight elongation in its shape, falling somewhere between round and cigar-shaped. The color indices suggest a relatively older stellar population with a lower rate of star formation. No signs of major mergers or significant tidal disturbances are evident, though there are some minor signs of disturbances in the image.
