The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge and a diffuse halo. The core exhibits a yellowish-white hue, suggesting an older stellar population. There is evidence of some disturbed features on the outer edges of this galaxy. One area appears to be extended outward suggesting a potential tidal tail or minor disturbance possibly due to a merging event. Overall, the galaxy appears moderately massive, with an observable star formation rate that would be considered low compared to actively star-forming galaxies. 
