The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. The color appears to be somewhat uniform, with a yellow-white hue dominating the central region, suggesting an older stellar population. There is little to no evidence of distinct spiral arm structures or prominent dust lanes. The galaxy's light profile seems to fade gradually from the core outwards, indicating a lack of significant ongoing star formation. Overall, the visual characteristics of this galaxy suggest it is a relatively evolved system, likely an elliptical or lenticular galaxy with a high degree of central concentration. No significant signs of interaction or disturbance are readily apparent.
