The galaxy presents as a spiral type, viewed at a moderate angle relative to its disk plane. A prominent central bulge dominates the inner region, exhibiting a bright, concentrated luminosity profile. Tightly wound spiral arms emanate from the bulge region, displaying a mottled texture indicative of star formation regions. A strong bar-like structure appears to traverse the central bulge. Dust lanes are visible along the inner edges of the spiral arms, obscuring some of the starlight. The overall color suggests a relatively evolved stellar population, though pockets of bluer light imply ongoing star formation. The galaxy shows no obvious signs of major mergers or strong tidal interactions, although there is some sign of a minor disturbance.