The galaxy presents a smooth, elliptical morphology. Its overall shape is elongated, appearing somewhat cigar-shaped, suggesting it is not perfectly spherical. The light distribution is concentrated towards the center, exhibiting a bright, relatively homogenous bulge. There's a gradual fading of light intensity from the core outwards, with no distinct spiral arm structures or prominent dust lanes visible. The galaxy's color appears generally consistent, with a slightly redder hue overall, indicating an older stellar population and low star formation activity. There appear to be no significant signs of ongoing or recent major merger events, such as tidal tails or strong morphological distortions, although there is a slight asymmetry present. 
