The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light profile. Its shape appears somewhat elongated, deviating slightly from a perfect circular form. The central region shows a brighter, more concentrated luminosity, suggesting the presence of a galactic bulge. The color profile indicates a generally older stellar population, with a yellowish-red hue dominating the central region and a more blue-ish hue on the outskirts. There appears to be an absence of prominent spiral arms or distinct dust lanes. Faint, disturbed features are subtly visible, potentially indicating a minor interaction with another galaxy or past merger event.
