The galaxy presents as a generally smooth, elliptical object with a concentrated central bulge. The core region displays a yellowish-white hue, indicative of an older stellar population. There is some apparent elongation, suggesting a morphology that is more lenticular than perfectly spherical. Faint traces of a disk-like structure are potentially present, though these are subtle and lack distinct spiral arms. No major disturbances or clear signs of ongoing merger activity are discernible within the limitations of the image quality. The galaxy's overall colour suggests moderate star formation activity, possibly confined primarily to the disk if present, as the bulge appears to be dominated by older, less active stars.
