The galaxy presents as a single, diffuse object with a dominant spheroidal morphology. The central region exhibits a bright, concentrated luminosity gradient, suggesting a high stellar density. A smooth, elliptical shape is apparent, with no distinct spiral arms or bar structures visible. Color gradients are subtle; the core appears slightly more yellow, transitioning to redder hues in the outer regions. The overall visual impression is that of a relatively quiescent galaxy, possibly an elliptical or S0 type, with a smooth stellar distribution and minimal ongoing star formation.
