The galaxy presents a predominantly smooth morphology, with a concentrated central bulge that exhibits a yellowish hue, suggesting a population of older stars. The overall shape appears to be somewhat elliptical, leaning towards being in between round and cigar shaped rather than distinctly circular. There is no clear evidence of prominent spiral arms or a well-defined disk structure. The outer regions of the galaxy fade gradually into the background sky, indicating a diffuse halo. There is no visible evidence of major mergers or significant tidal disturbances, suggesting relative isolation or past stabilization. Based on the color, it appears to have relatively low levels of star formation.
