The galaxy presents a generally elliptical morphology, with a central bulge exhibiting a yellowish hue, suggestive of an older stellar population. Surrounding the bulge, there is a fainter, diffuse disk component, showing a bluer color, possibly indicating regions of more recent star formation. While there is no definitive spiral structure visible, subtle irregularities in the disk's light distribution might imply some faint arm-like features or tidal disturbances. The galaxy appears relatively undisturbed, with no clear signs of a major ongoing merger, but potentially shows indications of minor disturbances. Overall, the galaxy exhibits intermediate luminosity, with a mass likely comparable to that of the Milky Way.
