The galaxy presents a generally smooth, elliptical morphology. Its central region exhibits a concentrated, bright, yellowish-orange core, suggestive of an older stellar population. Moving outwards from the core, the galaxy shows a gradual decline in surface brightness. There is an apparent extension of light around the central core, indicating the presence of an extended stellar halo. The galaxy exhibits minimal evidence of spiral arm structures or significant dust lanes; it appears largely featureless beyond its central concentration and extended halo. The shape appears more rounded than elongated. There's no clear indication of major mergers or tidal disturbances. Overall, the galaxy appears to be a relatively evolved system.
