The galaxy presents a smooth, elliptical morphology, with a high degree of central concentration. The light distribution appears consistent with an older stellar population, exhibiting a yellowish hue concentrated towards the core and a redder tone towards the outer regions. The isophotes are generally elliptical, but some slight deviations from perfect ellipticity are observed, suggesting subtle irregularities in the galaxy's structure. There appears to be no evidence of spiral arms or a prominent disk. There are some hints of possible minor disturbances, but no clear evidence of a major merger event. The object is moderately luminous.
