The galaxy appears to be a relatively compact and luminous object. It presents a largely smooth, elliptical morphology with a high degree of central concentration. There is an absence of distinct spiral arm structures or prominent dust lanes. The color profile suggests the presence of an older stellar population, with a reddish-yellow hue dominating the galaxy's overall appearance. There is no obvious evidence of ongoing major merger activity or significant tidal disturbances, however there may be a very slight warping in the disk. The object appears slightly flattened, with an axis ratio indicating a deviation from perfect circularity.
