The galaxy presents as a generally smooth, centrally concentrated object. It appears elliptical in shape, with a high degree of roundness, showing no obvious spiral arm structures or a prominent disk. The galaxy exhibits a color gradient, transitioning from a yellowish core to slightly greener outer regions, suggesting the presence of different stellar populations. The relatively smooth appearance indicates the absence of ongoing major mergers, though some subtle irregularities might indicate minor past interactions. It seems to be a fairly evolved system, with a significant fraction of older stars and a low rate of current star formation. The color is consistent with a population of aging stars and minimal dust obscuration.
