The galaxy presents as a slightly elongated, elliptical structure with a smooth, relatively featureless appearance. It displays a concentrated central bulge, characterized by a yellowish hue suggesting an older stellar population. The outer regions of the galaxy transition to a more diffuse bluish color, potentially indicating the presence of younger, hotter stars, or ongoing star formation, albeit at a relatively low rate. The galaxy lacks any obvious spiral arm structures or significant dust lanes. The overall morphology suggests a galaxy undergoing a transition from a spiral to an elliptical type, or a dwarf galaxy where star formation has not led to the formation of defined spiral arms.
