This galaxy exhibits a generally smooth morphology, displaying characteristics of an elliptical galaxy. Its shape is not perfectly round, presenting as somewhat elongated or cigar-shaped. There is a central concentration of light suggesting a bulge, with a gradual decrease in luminosity towards the outer edges. The galaxy presents a yellowish-white hue, possibly indicative of an older stellar population with lower star formation rates. There is little evidence of spiral arms or significant dust lanes, further supporting the classification as an elliptical galaxy. A hint of disk structure may be present, but is not clearly defined. The galaxy appears to be relatively isolated, with no obvious signs of major interaction or merging events. A small feature, possibly a minor disturbance, can be observed which is not highly defined.
