This galaxy exhibits a relatively smooth, elliptical morphology. The light profile is concentrated towards the center, with a gradual decrease in intensity towards the outer regions. The galaxy presents a yellowish-white hue, suggesting an older stellar population. The isophotes appear generally rounded, showing minimal signs of significant tidal disruption or interaction with other galaxies. There is a hint of redder colors around the edge of the galaxy, possibly indicative of a difference in the age of the stellar populations present in that part of the galaxy. No obvious spiral arm structures or prominent dust lanes are visible. The galaxy exhibits a notable red shift suggesting it is far away from the milky way. The rate of star formation within the galaxy is subdued. Overall, the galaxy appears to be a well-defined elliptical galaxy with a lack of features associated with active star formation or recent mergers.
