The galaxy presents as a smooth, elliptical-like object with a concentrated central bulge. The light distribution appears relatively uniform and decreases smoothly from the core outwards, which indicates a lack of prominent spiral arms or distinct features. The shape is elongated, with the ratio of the major to minor axis suggesting it is not perfectly spherical. There is no evidence of recent or ongoing major merger activity, although slight distortions cannot be entirely ruled out. The object emits primarily in the redder bands, indicative of an older stellar population and subdued recent star formation.
