The galaxy presents a generally smooth, elliptical morphology. Its light is concentrated toward the center, with a relatively featureless appearance beyond this central region. The color profile indicates the presence of older stellar populations, with light shifting toward the redder end of the spectrum. The galaxy exhibits a slightly elongated shape but does not appear to have strong disturbances or tidal features indicative of a major merger event. There is a hint of an internal structure but no clearly defined spiral arms or a prominent disk. The light is mostly concentrated near the center. No intense star-forming regions are visible in this imagery.
