The galaxy presents as a luminous, centrally concentrated object with an overall smooth morphology. The core region exhibits a bright, yellowish-orange hue, suggestive of an older stellar population. This color likely indicates the presence of evolved stars such as red giants and supergiants. The isophotes appear generally elliptical with a moderate ellipticity, neither perfectly round nor highly elongated. There are no discernible spiral arms or prominent dust lanes. Faint and diffuse extensions appear to emanate from the central region, fading gradually into the background sky. These extended regions exhibit a slightly bluer color than the core, hinting at a potential contribution from younger, hotter stars though the overall star formation activity is low. The overall structure suggests a massive galaxy, likely an elliptical or lenticular type. There is a subtle hint of minor gravitational disturbance, perhaps indicating a past interaction or minor merger event, but this is not definitive.
