The galaxy presents an elliptical morphology, elongated in shape. The light distribution appears relatively smooth, with a concentration of luminosity towards the center, suggesting a prominent bulge. Color gradients indicate potentially older stellar populations dominating the central region, which is a yellowish hue. Fainter blue regions appear around the edge of the galaxy, hinting towards areas of more recent star formation. No distinct spiral arms or prominent dust lanes are visible. The overall structure suggests a relatively evolved system. There is no clear evidence of interaction or significant disturbance in the galaxy's morphology.