The galaxy presents a generally smooth morphology, with a dominant central bulge that emits strongly in the yellow-red wavelengths. There's evidence of a disk structure, although it is relatively faint and not particularly well-defined. The overall shape appears elliptical, deviating slightly from perfect circularity but not exhibiting a pronounced cigar shape. There is a slight indication of some minor disturbance in the galaxy's structure, such as a possible warp or slight asymmetry in the outer regions, but no major merging event or strong tidal features are readily apparent. Based on the color, it is likely that the galaxy is populated primarily by older stars and the star formation rate is comparatively low.
