The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth light distribution with minimal discernible spiral arm structure or dust lanes. It is somewhat elongated in shape, more so than a perfect circle, but not severely so. The core exhibits the highest surface brightness, with a gradual decrease in luminosity towards the outer regions. The color profile suggests a population of older stars, as indicated by the yellowish-red hue across the galaxy, a sign of low star formation. There is no prominent tidal disturbance observed, suggesting no recent major mergers or interactions. 
