The galaxy presents as a slightly inclined disk galaxy. A central bulge is apparent, exhibiting a yellowish-orange hue. The disk surrounding the bulge shows hints of spiral structure, with bluish regions indicating areas of potential star formation. Overall, the galaxy appears relatively smooth in texture, although some minor disturbances may be present in the outer regions of the disk, potentially indicating recent or ongoing interactions. The color gradient suggests the presence of varying stellar populations throughout the galaxy, with older, redder stars concentrated in the bulge, and younger, bluer stars populating the spiral arms. The galaxy's moderate size and luminosity suggest a relatively substantial stellar mass.