The galaxy presents as a centrally concentrated object, exhibiting a relatively smooth morphology. There is a prominent, bright central bulge that appears roughly spherical. Surrounding the bulge, there is a fainter, more diffuse disk component. Hints of spiral structure may be present but are not clearly defined. The overall color of the central region leans towards yellow, with a shift to bluer hues as we look further out into the disk, indicating that the central bulge has older stars and the disk has younger stars. There is little evidence of significant ongoing star formation, nor significant tidal disturbances or interactions with neighboring galaxies. It displays a structure that is in between round and cigar-shaped.
