The galaxy presents an elliptical morphology, exhibiting a smooth, diffuse light distribution. The central region appears to be more concentrated, with a gradual decline in surface brightness towards the outer edges. The color profile suggests a dominance of older stellar populations, contributing to the observed yellowish hue. No distinct spiral arm structures or prominent dust lanes are visible. There is a slight asymmetry with minor disturbances, however this galaxy appears to be in a relatively undisturbed state.
