The galaxy presents as a disk-shaped system, oriented approximately edge-on to our line of sight. The central bulge exhibits a smooth, concentrated light profile, displaying a yellowish-white hue indicative of an older stellar population. This contrasts with the fainter, more diffuse disk component, which is elongated along the horizontal axis. There is some indication of features along the edges, hinting at a possible disk structure, but these are not well-defined. The color of the disc tends towards the red end of the spectrum, and a large portion of the light is centered around the center bulge. There are minimal signs of dust lanes or spiral arm structures. Overall, the galaxy appears to be a relatively quiescent system, although it is unclear if any weak star formation is happening within.
