The galaxy presents as a fairly smooth, elliptical structure with a noticeable central bulge. The luminosity appears to be concentrated in the core, gradually decreasing towards the outer regions of the galaxy. The shape is elongated, deviating from a perfect circle. The color profile suggests a population of older stars dominating the light output, with a redder hue. There may be limited signs of ongoing star formation, which is also evident from the lack of blue color. The galaxy does not show any obvious signs of tidal disturbances or mergers, exhibiting a relatively undisturbed morphology. There are hints of a faint halo.
