The galaxy appears as a relatively smooth, elliptical-like object with a concentrated central bulge. Its overall color profile leans towards the redder end of the spectrum. Faint diffuse light extends outwards from the central region, gradually fading into the background. There are no obvious spiral arm structures or dust lanes visible. The galaxy's morphology suggests it is likely a massive, evolved system, potentially with a moderately high stellar mass and a low rate of star formation. There are no indications of any ongoing major merging events, though there is a small chance of minor tidal disturbances. The isophotes appear roughly elliptical, though with some degree of irregularity. The galaxy is neither perfectly circular nor greatly elongated.
