This galaxy presents as a smooth, elliptical-like structure with a noticeable concentration of light toward the center, suggesting a prominent bulge. There is very little evidence of spiral arm structures or other distinct features. The galaxy appears to be relatively isolated, with no obvious signs of tidal disturbances or ongoing major mergers. The overall color is moderately red, indicative of an older stellar population, although there appears to be some bluer light present, possibly indicative of regions of recent star formation. The shape is somewhat elongated, not perfectly spherical, with hints of a flattened structure. There is a lack of pronounced dust lanes.
