The galaxy presents as a generally smooth, elliptical form, elongated in shape. It has a concentrated central bulge that emits primarily in the red-yellow spectral range, indicative of an older stellar population. The overall light distribution is centrally concentrated with no distinct spiral arm structures visible. Faint extensions of light may be present along the major axis but are poorly resolved in this image. There are no obvious signs of tidal disturbances or a major merger event. The disk appears relatively undisturbed.
