The galaxy presents as a central, concentrated luminosity with a slightly diffuse surrounding halo. The core appears largely smooth in texture, lacking any prominent spiral arm structures or distinct morphological features within the immediate vicinity of the galactic center. The light profile appears to be relatively uniform, with a subtle color gradient towards the outer edges. There is a lack of significant dust lane presence or knots of intense star formation. The galaxy is moderately elliptical. There is no evidence of any major merger events or significant tidal disturbances affecting the overall morphology.
