The galaxy presents as a smooth, elliptical form. Its overall shape is elongated, appearing cigar-shaped. There is a bright, concentrated central bulge that fades gradually into the outer regions of the galaxy. The color profile suggests older stellar populations. There is a lack of distinct spiral arm structures or irregular features, indicating a low rate of ongoing star formation. There is no obvious evidence of tidal disturbances or interactions with neighboring galaxies. The overall light distribution is consistent with an evolved, massive galaxy.
