The galaxy appears as a relatively smooth, centrally concentrated object with a slightly elliptical shape. There is minimal evidence of spiral arm structure or significant disk-like features. The light profile suggests a gradual decline in intensity from the core outwards, exhibiting an intermediate level of roundness, neither perfectly spherical nor highly elongated. Based on its overall morphology and lack of significant disturbances, it appears to be a relatively undisturbed system. The galaxy displays a blue hue, hinting at the presence of a young to intermediate stellar population. The object shows a star formation rate that is below average for galaxies of similar mass, indicating a quiescent period. Mass estimates suggest a relatively low mass galaxy.
