The galaxy presents a largely smooth morphology, with a significant central bulge of concentrated light that dominates the visual appearance. A surrounding disk is either absent or only faintly defined. The galaxy exhibits a roughly circular shape, with minimal elongation or asymmetry. The galaxy's color profile suggests a relatively older stellar population, with light tending towards the redder end of the spectrum. There is no clear indication of active star formation, although faint blue regions are present in areas that extend beyond the central bulge. No significant disturbances or signs of recent merger activity are observed. The galaxy appears relatively isolated and undisturbed.
