The galaxy presents as a centrally concentrated, luminous system with an overall elliptical morphology. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. Moving outward from the nucleus, the color transitions to a slightly bluer shade, indicative of some ongoing or recent star formation within the galactic disk. The galaxy appears relatively smooth in texture, with no prominent spiral arms or bar structures readily apparent. The edges of the galaxy fade gradually into the background sky, without any sharp discontinuities, which suggests a diffuse outer halo. There may be some very minor disturbances, but these are not very visible. The approximate luminosity is around -20 in the r band. This galaxy appears to be in a relatively isolated region of space.
