The observed galaxy presents a roughly elliptical morphology with a centrally concentrated luminosity profile. The core region exhibits a bright, high-intensity emission, suggesting the presence of a significant central mass concentration, potentially a supermassive black hole actively accreting material. Moving outward from the core, the galaxy displays a diffuse, extended halo.

The galaxy appears largely smooth, with limited evidence of distinct spiral arm structures or prominent dust lanes. However, subtle asymmetries and irregularities in the outer regions hint at possible gravitational interactions or past merger events. There appears to be a slight color gradient, with the central region exhibiting a bluer hue relative to the more reddish outer regions. This suggests a potentially younger stellar population in the core, potentially indicating recent star formation activity. Small, faint tidal features may be present but are not clearly defined. Overall, the galaxy appears to be a relatively mature system, though not completely without signs of past disturbances.
