The galaxy presents a relatively smooth, elliptical morphology. There is a bright, concentrated central bulge exhibiting a yellowish-orange color, suggestive of an older stellar population. Moving outward from the center, the galaxy fades in intensity. The outer regions appear more diffuse and less structured than the core, with a subtle color gradient indicating a possible transition in stellar populations. There is no apparent evidence of spiral arms or a prominent disk structure. The overall shape is largely circular, exhibiting slight ellipticity. There is no obvious sign of ongoing major mergers or tidal disturbances. The integrated color suggests a galaxy with a passively evolving stellar population and a low star formation rate.
