The galaxy presents as a relatively smooth, elliptical morphology. Its core exhibits a high degree of luminosity, with a color gradient shifting towards redder wavelengths from core to periphery. There is a notable absence of clearly defined spiral arms or significant dust lanes. The overall shape appears generally rounded, with a slight deviation towards a more elongated form. There is no evidence of recent or ongoing major merger events, although subtle irregularities in the outer halo may indicate minor disturbances. The observed color suggests a dominant population of older stars and a low rate of current star formation. Based on apparent size and color, this is likely a massive galaxy at a considerable distance.
