The galaxy presents a generally smooth, elliptical morphology with a central bulge that is bright and concentrated. The light profile indicates a centrally dominant stellar population, potentially an evolved one as the color appears slightly redder toward the core. There is no discernible spiral arm structure or prominent dust lanes. The overall shape is somewhat elongated, not perfectly spherical, suggesting a degree of ellipticity. The outer regions of the galaxy fade gradually into the background sky, lacking sharp edges or tidal features, indicating a relatively quiescent and undisturbed system. There is no strong evidence of ongoing major merger activity; however, subtle disturbances within the light distribution may suggest minor interactions in its past.
