The galaxy presents as a non-distinct elliptical, or possibly a spiral galaxy viewed at an angle. The galaxy exhibits a bright, concentrated central bulge with a yellowish hue, suggesting a population of older stars. Surrounding the central region, a fainter, somewhat diffuse disc-like structure is apparent, with hints of bluer regions, possibly indicating areas of more recent star formation. The overall morphology appears relatively smooth, with a small amount of disturbance, indicating no major merger events are taking place.
