The galaxy presents as a moderately luminous object with an overall elliptical morphology, though exhibiting features suggestive of a disk component. The central region displays a higher concentration of light, appearing as a bright, yellowish core indicative of an older stellar population. Extending outwards from this core, a fainter, bluer disk is discernible, though not sharply defined. There is no clear spiral arm structure visible. There may be some disturbances in the shape, which could potentially be indicative of a minor merger event, but the overall structure is mostly undisturbed. The galaxy is not viewed edge-on.
