The galaxy presents as a disk galaxy, seen at a slight inclination relative to our line of sight. The central bulge is prominent and appears relatively bright, suggesting a high concentration of older stars. Faint spiral arms are visible extending from the central region, indicating ongoing star formation. The galaxy is slightly elliptical in shape. The color suggests a mix of stellar populations, with the bulge exhibiting a yellower hue associated with older stars and the spiral arms showing bluer regions indicative of younger, hotter stars. There is no obvious signs of a major merger. The galaxy seems to be relatively undisturbed.