The galaxy presents as a moderately inclined disk system. It exhibits a concentrated central bulge, transitioning smoothly into a less defined disk. The central region displays a yellowish-orange hue, suggesting an older stellar population. Moving outwards, the disk shows a bluer tint, indicative of younger stars and ongoing star formation. The galaxy’s form is not perfectly circular; it presents an ellipsoidal shape. There may be minor disturbances in its structure, possibly due to minor gravitational interactions. The galaxy is primarily a smooth system, and no obvious spiral arm structures are visible. The light distribution is not entirely uniform, but is generally smooth.
