The galaxy presents as a disk galaxy, viewed nearly edge-on. A prominent bulge dominates the central region, exhibiting a smooth, rounded profile. The disk appears relatively thin and elongated, suggesting a high inclination angle relative to our line of sight. The bulge exhibits a yellowish-orange hue, possibly indicative of an older stellar population. The disk shows hints of bluer colors, particularly at its outer edges, suggesting ongoing star formation. There are some minor disturbances within the disc itself. There is no evidence of a strong tidal interaction or ongoing merger.
