The galaxy presents an overall elliptical morphology, appearing largely smooth and relatively featureless. There is a concentrated central bulge that appears to be the brightest region. Moving outwards, the galaxy shows a gradual decrease in luminosity, lacking sharp boundaries or distinct spiral arm structures. The color profile suggests a dominant population of older stars, exhibiting a yellowish hue with a slight red tint. There is no substantial evidence of active star formation regions, or dust lanes within the galaxy. It is likely a galaxy with a relatively low star formation rate and likely has a stellar mass that is on the higher end. No clear signs of ongoing major merger activity are apparent, such as tidal tails or significant morphological disturbances. Some asymmetry could point toward a potential minor disturbance. 
