The galaxy presents a generally smooth, elliptical morphology. It appears relatively compact, with a concentrated central region. The light distribution is largely uniform, lacking prominent spiral arms or distinct features. There is a subtle elongation, deviating slightly from a perfectly circular shape. The galaxy's color suggests an older stellar population, with a redder overall hue. There is no evidence of ongoing major merger activity or significant tidal disturbances in its immediate vicinity, though some minor asymmetries cannot be ruled out. The overall structure is suggestive of a relaxed system, nearing the end of its evolutionary timeline.
