The galaxy exhibits a largely smooth morphology, with a high degree of central concentration. Its shape appears generally round, with no obvious disk-like structure or prominent spiral arms visible. The color gradient suggests an older stellar population, with a yellowish-orange hue dominating the central region, potentially indicative of evolved stars and a lower rate of ongoing star formation. There is little evidence of significant dust lanes or recent merger activity influencing the galaxy's overall structure, however there are slight disturbances. Overall, the observed characteristics point toward a relatively evolved system that is trending towards a more quiescent state.
