The galaxy presents a roughly elliptical morphology, exhibiting a centrally concentrated luminosity profile. The core region is bright and appears relatively smooth with a yellow-white hue. Fainter, diffuse extensions emanate from the central region, displaying subtle color variations. A hint of bluer, less structured regions are visible outside of the main core, indicating the presence of star forming regions. There is evidence of possible tidal features or asymmetries suggestive of past interactions or ongoing merger activity. The galaxy appears somewhat disturbed, lacking a clear, symmetric disk structure. There are hints of arm-like structures, but these are faint and indistinct. Overall, the galaxy's light is dominated by older stellar populations with some regions of more recent star formation.
