The galaxy presents as a somewhat elliptical, smoothly distributed light source. Its core region exhibits a higher concentration of luminosity, appearing nearly spherical and emitting primarily in the redder wavelengths. Moving outward from the core, the galaxy displays a gradual decrease in surface brightness with a more irregular shape. There is little evidence of distinct spiral arms or prominent dust lanes. Faint bluish tints are observed in the outer regions, potentially indicative of younger stellar populations relative to the core. Overall, the galaxy appears to be a relatively undisturbed system, exhibiting features consistent with a massive galaxy at intermediate redshift and suggests a relatively low rate of star formation.