This galaxy exhibits a relatively smooth morphology, appearing largely featureless at this resolution. The light distribution is centrally concentrated, with a noticeable bulge region that emits prominently in yellow-orange wavelengths, suggesting an older stellar population. The overall shape is round, showing minimal signs of distortion or asymmetry. There is no discernible spiral structure or a clear disk component. The outer regions fade gradually, indicating a smooth transition in stellar density. A possible minor disturbance is visible on the outskirts of the galaxy on the right side, indicating a very possible gravitational interaction with a smaller object. Based on the apparent color and smoothness, this galaxy may be classified as an elliptical galaxy, potentially of significant mass. The galaxy shows signs of weak star formation activity overall.
