Observed is a galaxy with an apparent smooth morphology, appearing elliptical or lenticular. It presents a concentrated central bulge that dominates the galaxy's overall light output and contributes significantly to its mass. There may be a disk component, but it is difficult to confirm this as the disk is presented face on. The galaxy exhibits a yellowish hue overall, indicating an older stellar population with relatively low ongoing star formation, supported by a low star-formation rate. There is no clear indication of any major disturbances from merging events, and the overall shape suggests the galaxy is relatively relaxed. The estimated half-light radius is a few kiloparsecs, suggesting it is a galaxy of reasonable size, and the luminosity of the galaxy is quite bright. The estimated mass is quite high, indicating this is a massive galaxy.
