The galaxy presents an elliptical morphology, appearing largely smooth and featureless. Its color profile indicates a dominant population of older stars, exhibiting a reddish-yellow hue. A central bulge is evident, demonstrating a concentration of light. The galaxy appears relatively isolated, with no obvious signs of tidal interaction or ongoing merger activity, although subtle disturbances cannot be entirely ruled out due to image resolution. The overall shape suggests a relatively settled and evolved system, likely with minimal ongoing star formation.
