The galaxy presents as a somewhat elliptical structure with a centrally concentrated luminosity profile. The core region exhibits a bright, nearly uniform color indicative of older stellar populations. The surrounding disk shows a smooth, diffuse quality, fading gradually from the center. There is some evidence of a possible faint spiral arm structure beginning to form. One side of the disk shows a bluer color with a slight enhancement which might indicate some recent or ongoing star formation activity. The overall appearance suggests a galaxy that may be transitioning between an elliptical and a spiral morphology, or potentially a disrupted galaxy with a disturbed morphology but generally smooth features. There appears to be a ring like structure within the galaxy. This ring may be a site of dust absorption or intense star formation. There are no obvious signs of major mergers or tidal features, but some minor disturbance may be present based on the overall shape.
