The galaxy appears as a centrally concentrated, relatively smooth object. Its core exhibits a high degree of luminosity, suggesting a significant concentration of stars and potentially an active galactic nucleus. The light distribution falls off gradually from the center, with hints of a faint, extended halo surrounding the brighter central region. There are suggestions of some possible faint spiral arms. Color variations within the galaxy are subtle, but there is a general shift from bluer hues in the core region to redder hues in the outer parts, possibly indicative of different stellar populations and ages. There are suggestions of some mild disturbance in the galaxy, however these are minimal.
