The galaxy presents an elongated, disk-like morphology, viewed nearly edge-on. A bright, concentrated central bulge dominates the core region. The disk appears relatively smooth, with a gradual fading in luminosity from the central bulge outwards. There is some indication of obscuring dust lanes near the mid-plane of the disk, although these features are not sharply defined. No prominent spiral arm structures or distinct star-forming regions are readily apparent in the disk. The overall color profile suggests a relatively evolved stellar population, with a lack of significant blue light indicative of ongoing, vigorous star formation. There is no obvious evidence of any recent major merger events or strong tidal disturbances in the galaxy's morphology. Some minor asymmetry or warping of the disk may be present, warranting further investigation.
