The galaxy presents as a single, relatively smooth object with a somewhat spheroidal shape. The central region exhibits higher luminosity, with color indices suggesting an older stellar population. The galaxy shows minimal indications of spiral arm structures or prominent dust lanes. There appear to be signs of a potential recent or ongoing merger event, as evidenced by slight asymmetrical distortions in the outer regions and tidal tail-like features. The object has a moderate redshift, indicating that it is not a nearby galaxy. The color profile of the galaxy suggests that the outer regions have a younger stellar population than its central bulge.