The galaxy presents a generally smooth, elliptical morphology, appearing largely featureless upon initial inspection. The light profile suggests a concentrated central bulge, surrounded by a more diffuse halo. The galaxy exhibits a yellowish-white hue in the center and has a small disk. No pronounced spiral arm structures or dust lanes are discernible, suggesting a relatively quiescent state. The object's round shape indicates that this is an elliptical galaxy. There is evidence of ongoing, albeit relatively low, star formation. The overall appearance indicates a fairly evolved system. The galaxy appears isolated, and there is no indication of merging events.
