The galaxy presents as a relatively smooth, elliptical structure, exhibiting a centrally concentrated bulge that appears yellowish in color. This suggests an older stellar population residing within the core. Moving outwards from the core, the galaxy transitions into a bluer halo. The shape is more akin to an oval, not perfectly spherical, but not so elongated to be cigar-shaped. There is no obvious evidence of spiral arm structure or significant dust lanes, and the morphology seems generally undisturbed, with no major signs of a recent merger or tidal interactions.
