The galaxy presents as a relatively smooth, elliptical structure. The dominant feature is a bright, concentrated central bulge exhibiting a yellowish hue, possibly indicative of an older stellar population. The overall shape appears round, lacking any significant elongation or distortion. There is faint blue light outside of the bulge that could signify star formation. No significant spiral arms or disk features are readily apparent. There is no evidence of a major merger event. There is minimal disturbance in morphology.
