The galaxy presents a generally smooth, elliptical morphology. Its light distribution is centrally concentrated, exhibiting a bright, slightly reddish core that gradually diffuses outwards. The overall shape is elongated, approaching a cigar-like appearance, with no distinct spiral arm structures visible. There's a subtle color gradient from the center towards the outer regions, transitioning towards a bluer hue, which suggests the presence of a younger stellar population in the outskirts compared to the more aged population concentrated in the core. There is no apparent sign of tidal disturbances or ongoing merger activity, and it appears undisturbed.
