The galaxy appears as a slightly elongated, diffuse object, exhibiting a centrally concentrated brightness profile. The core region displays a warmer color, trending toward yellow and orange, which may indicate an older stellar population. Surrounding this core, a fainter, bluish-green halo is visible, possibly indicating the presence of a younger stellar population or regions of ongoing star formation. The overall structure seems relatively undisturbed, lacking prominent spiral arms or tidal features, suggesting a relatively quiescent or undisturbed evolutionary history. The galaxy does not exhibit any obvious signs of active galactic nuclei activity or substantial dust lanes. The image resolution limits a more detailed morphological classification.
