This galaxy appears to be a relatively smooth, centrally concentrated object. There is a dominant central bulge that emits strongly in the green-red part of the spectrum, indicating an older stellar population. The galaxy exhibits a more diffuse, fainter halo, with some bluer color, hinting at a small amount of ongoing star formation in the outer regions. There are no obvious spiral arms or a disk-like structure visible at this resolution. The overall morphology suggests an elliptical galaxy, though not perfectly spherical, with a slight deviation from roundness. There is no obvious evidence of major mergers or significant tidal disturbances in the immediate vicinity. The estimated distance to the galaxy places it at a redshift of approximately 0.13.
