The galaxy appears to be a relatively smooth, elliptical type, exhibiting a centrally concentrated bulge. The core region shows a yellowish-red hue, indicating a population of older stars and a lower rate of ongoing star formation. There is a subtle flattening, suggesting a potential deviation from a perfectly spherical shape. Weak, extended outer regions appear with faint blue tinges implying some small amount of recent star formation. There is no apparent spiral structure or significant dust lanes visible in this image. No signs of major mergers or tidal disturbances are immediately apparent. The overall impression is that of a mature, quiescent system.
