The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth and rounded morphology. It has a discernible central bulge that is bright and concentrated, with the rest of the galaxy appearing to fade outward, forming a halo of light. The galaxy's color is dominated by redder hues, suggesting a stellar population that is relatively old, and a lower rate of active star formation. There is a slight hint of a disk structure, but it's not particularly prominent, with no clear spiral arms visible. The overall structure appears relatively undisturbed, without signs of major mergers or significant tidal interactions. There's a slight asymmetry in the outer regions suggesting a possible minor disturbance or interaction.