The galaxy presents a smooth, elliptical morphology. It appears elongated, with a noticeable cigar shape. The galaxy's color gradient suggests a primarily older stellar population, with a yellowish hue dominating the central region. The light distribution is relatively uniform across the galaxy, lacking distinct spiral arm structures or prominent star-forming regions. There is no indication of any significant ongoing merger activity or major disturbances in its structure. There are no visible dust lanes or distinct features to suggest recent interactions or significant gas content. Overall, the galaxy appears to be a relatively evolved system with a low rate of star formation.
