The galaxy presents as a somewhat smooth, rounded structure. There is no distinct spiral arm morphology visible. The color appears yellowish-white, with a concentration of brighter, perhaps older stars within the central region. There is some subtle evidence of a disk structure, with the galaxy being less concentrated on one end. The lack of distinct features, such as prominent dust lanes or star-forming regions, suggests a relatively low current star formation rate. There is no evidence of a major ongoing merger, although the irregular appearance of one side of the galaxy suggests a possible tidal interaction.
