The galaxy presents as a relatively smooth, elliptical-like structure with no discernible spiral arms or a distinct disk component. It exhibits a concentrated, bright central bulge, which gradually diffuses outwards. The overall color profile appears to be predominantly yellow, suggesting an older stellar population. There is some evidence of bluer hues on the periphery, indicative of more recent or ongoing star formation in the outer regions, though this is minimal. No significant tidal features or signs of a recent merger are immediately apparent. The galaxy has an estimated size of roughly 4 kpc, with a mass estimate of 10^10 solar masses. The star formation rate is relatively low. The galaxy displays a high degree of central symmetry and does not appear to be heavily disturbed.
