The galaxy appears to be elliptical in morphology, exhibiting a generally smooth light distribution. The central region displays a high concentration of light, gradually decreasing in intensity outwards. There is a slight elongation, indicating a deviation from perfect circularity, but it's closer to being round than cigar-shaped. The color profile suggests a predominantly older stellar population, leaning towards redder hues in the core, shifting towards bluer hues in the surrounding regions. No spiral arm structures or significant dust lanes are discernible. There are subtle hints of minor disturbances or tidal features in the outer halo, though the structure is dominated by its elliptical form. There is no evidence of it being an ongoing major merger.
