The galaxy presents a generally smooth morphology, exhibiting a concentrated central bulge that radiates strongly in the yellow-red part of the spectrum. This central region transitions into a less luminous, more diffuse halo exhibiting a greenish hue. The galaxy's shape appears to be somewhat elliptical, leaning toward a circular form. There is no visually apparent evidence of a distinct disk structure, major mergers, or strong tidal disturbances. Minor disturbances cannot be ruled out, though the system appears dynamically relaxed. Star formation appears low, suggested by the lack of bright blue regions typically associated with younger stellar populations.