The galaxy presents as an elliptical-like structure with a bright, concentrated central bulge. The bulge exhibits a yellow-orange hue, suggesting an older stellar population. Surrounding the bulge is a fainter, more diffuse disk. This disk appears relatively smooth with subtle variations in brightness, hinting at possible spiral arm structures, although they are not clearly defined. The disk color appears slightly bluer than the central bulge, indicating the presence of younger, hotter stars. There is no obvious sign of recent or ongoing major merger events. The galaxy exhibits a moderate redshift. Overall star formation appears low. The galaxy is roughly 4 kiloparsecs in size.
