The galaxy presents as an elliptical morphology, appearing somewhat flattened but primarily smooth in structure. Its color profile suggests an older stellar population, exhibiting a yellowish-orange hue indicative of evolved stars. There is a slight concentration of light towards the galactic center but lacks a prominent core. Faint indications of minor disturbances are present, potentially suggestive of past or ongoing interactions, but these are not strongly defined. The galaxy does not present prominent spiral arm structures. Overall the image suggest a galaxy which has gone through past interactions, but is not currently undergoing any major merger.
