The galaxy presents as a central, concentrated spheroid with a yellowish hue, suggestive of an older stellar population. Emerging from this central region is a fainter, elongated structure that exhibits a bluer color. This blue component suggests the presence of younger, hotter stars and possibly ongoing star formation. The overall morphology appears disturbed, with an asymmetry in the distribution of light. The spheroid component appears relatively smooth, while the elongated structure is more diffuse and irregular. There may be some tidal interactions or a recent merger event. 
