The galaxy presents as an elliptical morphology with a relatively smooth light distribution. There is a high degree of central concentration indicated by a bright, somewhat diffuse core. The overall color profile appears to be trending towards the redder end of the spectrum, indicative of an older stellar population and a possible lack of significant recent star formation. There appears to be a slight irregularity to the shape, possibly due to a minor gravitational interaction or an internal structure not easily resolved at this scale. The overall appearance suggests a well-evolved system, characteristic of early-type galaxies.
