The galaxy presents a largely smooth morphology, exhibiting a high degree of circularity. There is no discernible spiral arm structure. The galaxy appears to be dominated by an elliptical shape, with the light distribution concentrated towards the center, suggesting a prominent bulge. Color gradients show a bluer hue in the outer regions and a yellowish-red core, indicating a potential difference in stellar population ages. The lack of any apparent tidal features or close companions suggests that this galaxy may be relatively isolated or has not recently undergone a major merger event. There may be some indication of a small amount of star formation activity. Overall, the galaxy appears to be a fairly evolved system, but the image quality limits further detailed analysis.
