The galaxy appears as a singular, generally homogenous object with a smooth morphology. The shape is largely circular, with minimal elongation. The galaxy's color profile exhibits a progression from a brighter, more yellow central region, diffusing outward into a reddish hue at the periphery. There is no indication of spiral arm structures or prominent dust lanes. The light distribution suggests a concentration of older stellar populations. It lacks visible signs of active star formation. There are no apparent distortions or tidal features indicative of ongoing or recent merger activity. The galaxy exhibits a consistent, blended color profile.
