The galaxy presents a generally smooth, elliptical morphology. A concentrated, luminous core exhibits a yellowish hue, suggestive of an older stellar population. Diffuse, fainter material surrounds the core, extending outwards in a somewhat elliptical distribution. This outer region shows subtle color variations, with hints of bluer tones intermixed with the dominant yellowish light, potentially indicating regions of ongoing, albeit low-level, star formation. The overall structure appears relatively undisturbed, lacking significant tidal features or evidence of recent major mergers. There may be minor disturbances present but they are very subtle. It's difficult to determine the exact shape and orientation of the galaxy due to the lack of clear spiral arm structures or a well-defined disk.
