The galaxy appears as a relatively smooth, elliptical-like structure with a bright, concentrated central bulge. The light distribution fades gradually from the center outwards. There is a very faint, diffuse disk component possibly present surrounding the bulge. There is a slight asymmetry to the galaxy's outer isophotes. No distinct spiral arms or prominent dust lanes are visible within this image. The galaxy's color is primarily a yellow-white hue, suggesting a relatively older stellar population, though the bluer color within the central bulge may suggest more active recent star formation there. There is no indication of ongoing major merger activity. Possible very faint disturbances are too difficult to verify from this image. Overall, the galaxy exhibits characteristics of a relatively evolved system.
