The galaxy exhibits a generally elliptical morphology, appearing elongated with a high degree of axis asymmetry. Its light profile seems to be fairly smooth, lacking prominent spiral arms or distinct features. Color gradients are subtle, showing a central concentration of yellowish-orange hues which could imply an older stellar population, towards a bluer, less concentrated halo of material that may contain pockets of ongoing star formation. There are faint hints of minor disturbances, likely due to a past merger or tidal interaction, but overall, it displays a fairly settled structure. The galaxy does not appear to be actively undergoing a major merger.
