The galaxy presents as a centrally concentrated object, with a largely smooth appearance. Its overall form is elliptical, exhibiting a high degree of roundness. There is a slight elongation to the shape, but not significantly cigar-shaped. A faint disk component is either absent or not readily discernible. The light distribution is concentrated towards the center, with a gradual decrease in surface brightness moving outwards. The object displays a yellowish hue, suggesting an older stellar population and a relative paucity of ongoing star formation activity. No clear signs of recent or ongoing mergers are present. Indications of minor disturbances are subtle at best, with the overall morphology appearing relatively undisturbed.
