The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that graduates outward into a fainter, more diffuse halo. The galaxy presents a slightly elongated shape, suggesting it is not perfectly spherical. It has a yellowish-red hue, indicative of an older stellar population and lower levels of on-going star formation. While a dominant spiral structure is not evident, there might be a faint hint of a disk, but it is not pronounced. No major tidal disturbances or signs of ongoing merging activity are immediately apparent. The morphological characteristics suggest it is a mature galaxy.