The galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution suggests a high degree of radial symmetry, though not perfectly spherical. A slight elongation is noticeable, giving it a more lenticular appearance. The color profile indicates a predominantly older stellar population, characterized by yellowish hues, with relatively little evidence of recent star formation. There are no distinct spiral arms or prominent dust lanes visible within the optical bands. Its structure is moderately compact. There are potentially tidal features visible at the very edge of the galaxy, indicating this galaxy could be undergoing or have undergone a recent minor merger. The outskirts of the galaxy gradually fade into the background sky, implying a smooth stellar density profile.
