The galaxy presents as a centrally concentrated system with a largely smooth light distribution. The core is bright, showing a bluish-white hue, indicative of possible recent or ongoing star formation in this region. Moving outwards from the center, the light appears more diffuse with slightly redder tones. The galaxy exhibits an overall roundness in its morphology with only slight irregularities hinting at minor gravitational interactions or internal disturbances. There is no clear evidence of spiral arm structure or a distinct disk component. Faint hints of tidal disturbances or asymmetry suggest the possibility of a minor merging event in the past or perhaps a low level of ongoing interaction.
