The galaxy appears to be an elliptical galaxy, characterized by a generally smooth, featureless morphology. It exhibits a slightly elongated shape, deviating somewhat from perfect circularity. The central region of the galaxy is notably brighter and more concentrated, suggesting a higher density of stars in the galactic nucleus. The color profile indicates a predominantly older stellar population. A faint reddish hue is detected in one of the outer arms, which indicates that there is some minor star formation activity occurring. There is no obvious evidence of spiral arms or a prominent disk structure, which supports the classification of this galaxy as an elliptical. There are also no obvious signs of a major merger event.
