The galaxy exhibits a primary, centrally concentrated component with a smooth, spheroid-like morphology, appearing largely featureless. This central region displays a yellowish hue, suggesting an older stellar population. A secondary, fainter component extends from the main body, exhibiting a bluer color, potentially indicating regions of younger star formation or a tidal tail resulting from an interaction. The overall structure shows signs of possible disturbance, with some asymmetry present. The shape of the main body is largely round. There also may be evidence of merger activity.
