The galaxy presents as a largely featureless, smooth elliptical structure. The central bulge exhibits a concentrated, luminous profile, indicative of a high stellar density. Moving outward from the core, the light gradually diffuses into a more extended halo. There is a slight elongation to the galaxy's shape, suggesting it may be of type E4-E5 on the Hubble sequence. The color appears generally red, with the galactic center appearing slightly more yellow-orange than the outer halo. There are no discernible spiral arms or dust lanes. The overall morphology is consistent with an older stellar population and low ongoing star formation. There is no visually apparent evidence of any tidal disturbances or ongoing mergers.
