The galaxy appears as a centrally concentrated object with a generally smooth profile, suggesting an elliptical or lenticular morphology. The central region exhibits a brighter, more intense luminosity. A slight elongation is observed, indicating that the galaxy is not perfectly spherical. There seems to be a slight disturbance or faint feature extending from the core. Based on the color distribution, there is a hint of bluer light surrounding the central bulge, which might indicate younger stellar populations.