The galaxy appears as a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge that gradually diffuses outwards. The light profile transitions smoothly from the bright core to the fainter outer regions, with no apparent spiral arm structures or significant dust lanes visible. Its overall shape is close to round with a slight elongation. The color distribution across the galaxy seems fairly uniform, with a yellowish hue dominant in the central region, indicating a population of older stars. There is no prominent, active star formation observed within the galaxy.
