The galaxy presents as a relatively smooth, elliptical morphology with a discernible central bulge. There is a slight elongation to the galaxy's shape, deviating minimally from a perfectly circular form. The color profile suggests a dominant population of older stars, indicated by the yellowish hue of the central region. Fainter blue-ish regions are slightly present in the extended area of the galaxy indicating the presence of younger stars, but most of the star formation has already occurred. A small fraction of the galaxy shows faint signs of tidal distortion and a slight asymmetry suggesting a possible minor interaction or merger event in its past. There is no strong evidence of active star formation visible, no spiral arms, and the galaxy appears to be evolved.
