The galaxy appears as a centrally concentrated object, exhibiting a roughly elliptical morphology. The core region is characterized by a bright, relatively smooth distribution of light, suggesting a significant population of older stars. Moving outwards from the core, the luminosity gradually decreases. The color of the galaxy shifts from a bright white/blue hue in the center, to a green hue around the core, and eventually a more red color at the edges of the halo. There is no significant spiral arm structure or presence of distinct dust lanes visible in the image. However, the faint extensions may indicate some level of tidal disturbance or ongoing interaction with another galaxy. Overall, the galaxy presents an appearance consistent with that of an early-type galaxy, potentially an elliptical or lenticular galaxy.
