The galaxy presents a generally smooth morphology, indicative of a relatively evolved system. A faint, diffuse disk is visible, hinting at some level of rotational support. Evidence suggests it is potentially undergoing a merger or has experienced recent gravitational interaction, with some visible distortions in its overall shape. The color gradient transitions from a bluer central region to redder outer regions, suggesting ongoing or recently ceased star formation, with the blue light indicating hotter, younger stars in the central region. Its absolute magnitude is in keeping with the size. The estimated mass is well within the range of an average galaxy.