This galaxy presents as an elliptical type, exhibiting a generally smooth and concentrated light profile. It is somewhat elongated in shape, with a cigar-like appearance, with no easily discernible spiral arm structure. The color appears to be a relatively uniform bluish-white throughout, which indicates that the stellar population is mostly older stars with some more recent star formation, though not as significant as what may be observed in more strongly blue spiral galaxies. There appears to be a bright central bulge, which is likely a supermassive black hole. There is no significant indication of a major merger event, but some minor disturbances cannot be ruled out.
