The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high degree of concentration, with a bright, yellowish-white core. The luminosity gradually decreases towards the outer edges of the galaxy, which appear somewhat diffuse and indistinct. There is little evidence of significant spiral arm structure or dust lanes. The overall color profile indicates a population dominated by older stars. There is a slight indication of a blueish hue at the edges, implying low levels of recent star formation. The galaxy's shape is generally round, with only a slight deviation from a perfect circle. There are no signs of major tidal disturbances or ongoing merging activity.