The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology with a high degree of symmetry. The light profile suggests a bulge-dominated system, with a noticeable lack of defined spiral arm structures. The color indices indicate a predominantly older stellar population, as evidenced by the redder hues throughout the galaxy's body. There is a suggestion of some recent star formation activity, with slight blue-ish tints. The overall appearance implies a relatively evolved system undergoing little to no current major merging events.
