The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. There is minimal evidence of distinct spiral arms or a prominent disk. Its overall shape tends towards round, with a slightly flattened appearance. Color gradients suggest a possible redder core region with bluer outer regions, perhaps indicative of older stellar populations concentrated centrally and younger populations towards the edges, though the effect is subtle. There is no apparent ongoing major merger activity, nor strong tidal disturbances, though there are some minor irregularities in the overall form. The galaxy displays an overall intermediate brightness, indicative of a moderately luminous object at its given redshift.
