The galaxy appears to be an elliptical type, exhibiting a smooth, diffuse light distribution. It presents with a generally rounded morphology with an average size. The central region shows a concentrated, brighter core that dims significantly in its outer regions. There may be a hint of a faint disk structure. There is a possible indication of a minor gravitational disturbance or tidal interactions in its morphology, with slightly asymmetrical light distribution or potential minor arm-like extensions. The color profile suggests a population of older stars, indicated by the redder hues, though some bluer light suggests possible star formation activity, albeit at a low rate. The galaxy shows no evidence of spiral arms or a bar.
