The galaxy appears as an edge-on spiral, presenting a clear disk structure viewed nearly perpendicular to its rotational axis. The central bulge exhibits a yellowish-orange hue, suggestive of an older stellar population. The disk shows bluer regions tracing the spiral arms, where active star formation is likely occurring. The dust lane bisects the galaxy along the equatorial plane. There are no signs of prominent tidal features or ongoing major mergers. The galaxy's morphology is consistent with a relatively undisturbed, late-type spiral system.
