The galaxy presents as a concentrated central region with a slightly elongated structure, possibly exhibiting a weak bar or disk-like component viewed at a shallow angle. The core appears bright and yellowish-orange, suggesting an older stellar population. Fainter, more diffuse green-tinged material surrounds the central bulge, potentially indicating ongoing, though subdued, star formation or the presence of ionized gas. There is an adjacent object which has a more compact and reddish-orange appearance, indicative of a more concentrated and older stellar population; it is not clear whether this is a secondary bulge within the galaxy itself, or if it is an adjacent companion galaxy. Based on the morphology, the galaxy likely resides towards the quiescent end of the star-formation spectrum, with its smooth appearance pointing to a relatively evolved stage of development, with only a modest degree of visible disturbance or recent merger activity.
