The galaxy appears to be relatively smooth in overall structure, with a bright, concentrated central bulge region. This suggests a significant population of older stars concentrated in the center. There is some evidence of a disk component, though it's not highly pronounced. The galaxy is generally elliptical in shape but not perfectly so; it is somewhere in between round and cigar shaped. There are indications of some internal structure within the galaxy, but no major signs of any merger activity or significant tidal disturbance. Faint blue colorations are observed in the surrounding area of the bulge, which suggests more active star formation.
