The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central region, suggestive of a substantial galactic bulge. The overall color appears to be somewhat redder, possibly indicating an older stellar population and a lower rate of ongoing star formation. There is little evidence of spiral arms or significant dust lanes within this resolution. The galaxy displays a high degree of symmetry with a shape that is somewhere between round and elongated. There is no indication of any major ongoing merging activity or significant tidal disturbances. The estimated size is around 6 kpc across.
