The galaxy presents as a spiral galaxy with a moderate inclination relative to our line of sight. A central bulge region is discernible, although not highly pronounced, and appears to be intermediate in size. The disk component of the galaxy exhibits faint spiral arm structures, some traces appear as brighter regions. A slight elongation suggests the possible presence of a bar feature. Overall, the galaxy's light distribution is relatively smooth, with limited indications of significant starburst regions or tidal disturbances, although a more careful examination is necessary to rule out faint features indicating past interactions.
