The galaxy presents a largely smooth, elliptical morphology with a high degree of roundness. There are no apparent spiral arm structures or significant disk-like features. The light distribution is centrally concentrated with a gradual fall-off in intensity towards the outer regions. The core exhibits a yellowish hue, possibly indicative of an older stellar population. The red shift measurements indicate that the galaxy is relatively far from our own. A very slight asymmetrical deviation from perfect roundness hints at a possible minor gravitational interaction but no clear merging activity is directly observed. The lack of strong blue emission indicates that the star formation rate may be relatively low. 
