The galaxy presents as a largely featureless, elliptical morphology. The light distribution appears smooth and concentrated towards the center, exhibiting a yellow-orange hue that suggests an older stellar population. A slight elongation is observed, deviating from a perfectly circular shape, with the major axis oriented roughly horizontally in the image. There's minimal evidence of spiral arm structures or dust lanes. The overall impression is that of a mature galaxy with low star formation activity. A faint, diffuse blue halo is barely perceptible around the main body of the galaxy, possibly indicating the presence of a small population of younger, hotter stars. No signs of significant tidal disturbances or ongoing merger activity are apparent.
