The galaxy presents as a relatively smooth, elliptical morphology with a high degree of central concentration. The light distribution is symmetrical, with no apparent spiral arms, bar structures, or prominent dust lanes. The color profile suggests a population of older stars, as evidenced by the yellowish-red hue, particularly in the core region. There is minimal evidence of recent star formation activity based on the absence of blue or ultraviolet light. The overall form appears relaxed, indicating it is unlikely to have undergone a recent major merger event. There might be some minor asymmetries. However, the dominant impression is of a well-formed, evolved system.
