The galaxy presents a flattened, elliptical morphology. It appears largely smooth in texture, lacking prominent spiral arms or strong indications of active star formation regions. The light distribution suggests a more or less homogenous stellar population. The central region exhibits higher luminosity, gradually fading towards the outer edges. The overall color is slightly bluish, indicating some presence of younger stars, but it is dominated by older stars. There is no obvious indication of recent merger events or significant disturbances in its structure, although there is a slight asymmetry on the right side of the galaxy. The galaxy does not appear perfectly circular; instead, it has an elongated shape, but it is closer to being round.
