The galaxy presents as a moderately luminous object exhibiting a relatively smooth morphology. It displays an elliptical shape, being somewhat elongated rather than perfectly spherical. The galaxy's color profile indicates a range of stellar populations, with a central region appearing more concentrated and having a bluer hue compared to the outer regions, which tend towards a redder color. There is some evidence of minor disturbances in its structure, possibly indicating past or ongoing interactions with other galaxies, though the overall structure remains largely undisturbed. No distinct spiral arms are discernible.
