The galaxy presents a smooth, elliptical morphology with a concentrated central bulge that exhibits a yellowish hue, indicative of an older stellar population. The overall shape appears somewhat elongated, deviating from a perfectly circular profile. There's a noticeable radial decrease in luminosity from the core outwards, suggesting a gradual transition to a fainter halo. There is no obvious disk component or spiral arm structure. The galaxy appears to be relatively undisturbed, without any prominent signs of ongoing merger activity or tidal distortions.
