The galaxy presents a largely smooth morphology, with a high degree of central concentration. Its overall shape appears to be somewhere between round and elliptical. There is a distinct lack of significant spiral arm structures or prominent dust lanes. The galaxy exhibits a color gradient, transitioning from a yellowish core to bluer outer regions. This suggests the presence of an older stellar population concentrated in the center, with younger stars residing further away. There is no strong indication of tidal tails or major morphological disturbances, suggesting the absence of recent major merger activity. However, a mild asymmetry in the outer regions hints at possible minor interactions. Overall, the galaxy's light profile seems to be well fit by a smooth profile, perhaps like a Sersic profile, without strong features. 
