The galaxy appears to be an elliptical morphology, viewed at a moderate inclination. Its shape is elongated, with an estimated axis ratio indicating a deviation from perfect circularity. A central bulge is present and prominent, with a concentrated luminosity profile. The disk component is present, but appears smooth without prominent spiral arm structures. The galaxy exhibits a color gradient, with the central bulge appearing yellower and the outer regions appearing bluer. This suggests a potential difference in stellar populations, with older stars concentrated in the bulge and younger stars residing in the disk. Overall, the galaxy's morphology indicates a transition from a pure elliptical to a lenticular type.
