The galaxy presents as an edge-on spiral, or possibly a lenticular, system. The central bulge is prominent, appearing bright and somewhat concentrated. The bulge is elongated along the major axis, and its color suggests an older stellar population, potentially with a lower rate of on-going star formation. The disk appears relatively thin and extended. Faint traces of blue light are visible along the outer edges of the disk, suggesting the presence of younger, hotter stars and possible regions of active star formation. There is no indication of significant dust lanes or morphological disturbances. The overall structure appears relatively smooth and undisturbed, with no clear signs of recent mergers or tidal interactions. The galaxy is characterized by a morphology dominated by a disk oriented edge-on relative to the observer's line of sight.
