The galaxy presents as a fairly smooth, elliptical morphology. There is no discernible spiral arm structure. The light distribution indicates a relatively even profile across the galactic body with the exception of the noticeably brighter core. The color profile appears relatively homogeneous, showing what appears to be a slightly yellow to red-shifted profile indicative of an older stellar population. There does not appear to be any signs of active merging events or major disturbances in its immediate vicinity. Its apparent shape is elongated but not extremely so, appearing slightly cigar shaped. From the color and smooth texture, this galaxy likely has a significant stellar mass and a moderate star formation rate.
