The galaxy presents as a relatively bright, elliptical object with a high degree of central concentration. Its overall color is dominated by a yellowish-white hue, suggestive of an older stellar population. The light distribution appears mostly smooth, with only subtle variations in surface brightness across the galactic disk. The shape is noticeably elongated, departing from a perfectly circular form; it exhibits a moderate ellipticity, appearing more disk-like than spheroidal. There is minimal evidence of distinct spiral arms or prominent dust lanes, indicating that this is most likely a mature galaxy, potentially an elliptical or lenticular type. There is no obvious indication of an active galactic nucleus or recent major merger activity, although a very slight asymmetry might hint at minor disturbances. The galaxy appears relatively isolated within the field, with no immediately interacting companion galaxies visible. The presence of some diffuse light extending beyond the main body of the galaxy suggests a gradual decline in stellar density with increasing radius.
