The galaxy presents an overall elliptical morphology, appearing as a relatively smooth, concentrated distribution of light. Its shape is not perfectly spherical, exhibiting a slightly elongated form. The central region is characterized by a bright, dominant core, suggesting a concentration of older stellar populations. Fainter, more diffuse light extends outwards from this core, exhibiting a gradual decrease in surface brightness. The color gradient appears subtle, with a suggestion of redder hues in the central regions compared to the bluer outskirts. The overall structure does not reveal prominent spiral arms or distinct features indicative of active star formation within the galaxy itself. There appears to be some minor disruption in the overall form on one side, suggesting possible past interaction with another galaxy.
