The galaxy appears as a relatively smooth, elliptical or spheroidal structure. Its light profile exhibits a centrally concentrated bulge, with a gradual decrease in luminosity outwards, indicating a lack of distinct spiral arms or a prominent disk component. The color appears to be generally yellow/orange, suggesting a population of older stars and a lack of significant ongoing star formation. There is no clear evidence of any major disturbances or tidal features suggesting a recent major merger event, although minor asymmetries could indicate past interactions. The galaxy exhibits a generally round shape, lacking a highly elongated or cigar-shaped morphology.
