The galaxy presents as a relatively smooth, centrally concentrated object. It appears to exhibit a predominantly elliptical morphology, with a slightly elongated shape. The central region displays a bright, concentrated core, suggesting a potential bulge or active galactic nucleus. There may be some subtle, faint features suggestive of a disk component or spiral arms, but they are not clearly defined. There is a minor likelihood of a merger based on the smooth form, but a major disturbance is possible. The galaxy is likely a few kiloparsecs in effective radius.
