The galaxy presents a largely smooth, elliptical morphology. The light distribution is concentrated towards the center, exhibiting a bright, unresolved nucleus. Proceeding outwards from the nucleus, the luminosity decreases gradually with no distinct spiral arm structure or prominent dust lanes visible. The galaxy appears mostly featureless, with a slight elongation in its overall shape. The color profile suggests an evolved stellar population, leaning towards redder hues, which supports the smooth morphology. There is no strong evidence of ongoing major mergers or tidal disturbances. The galaxy is relatively isolated.
