The galaxy presents as a flattened elliptical morphology, approximately 4 kpc in radius. There is a distinct color gradient from the center outwards. The central region appears a yellowish hue which transitions to a more bluish white at the periphery. This may be due to older stellar populations being concentrated in the galactic center, while younger stars are more common in the outer regions. The galaxy exhibits a smooth appearance overall, with no obvious signs of spiral arms or significant dust lanes. The aspect ratio of the galaxy suggests a significant inclination relative to the observer's line of sight. The shape is somewhat "cigar shaped," more elongated than a typical elliptical galaxy. The galaxy does not appear to be undergoing any major merging events, or experiencing significant tidal disturbances. Overall, this galaxy appears to be a relatively undisturbed, evolved system.
