The galaxy presents as a singular, relatively smooth object with a high degree of circularity in its morphology. The galaxy exhibits a concentrated, centrally luminous core, appearing largely spheroidal. There is some indication of slight color variation across the galaxy, with the central region appearing yellower, possibly indicating an older stellar population. The outer regions exhibit a slightly bluer hue, which could suggest the presence of younger stars. No distinct spiral arm structures or prominent dust lanes are apparent. The overall impression is of an elliptical or S0-type galaxy, exhibiting minimal signs of recent or ongoing merger activity or significant internal disturbances. The object is compact, without an extended halo. The moderate redshift suggests a relatively distant object. The estimated size suggests it is a reasonably sized galaxy.
