The galaxy presents a generally elliptical morphology, appearing somewhat elongated along a northeast-southwest axis. Its overall color profile suggests a mix of stellar populations, with a prominent central bulge exhibiting a yellowish hue, indicative of older, redder stars. Surrounding this bulge, a faint blueish halo or disk-like structure is visible, implying the presence of younger, bluer stars, and potentially ongoing or recent star formation, particularly in the outer regions. There is a suggestion of minor gravitational disturbance or tidal interaction occurring, with some asymmetry noticeable in the distribution of light in the outer halo. The relatively smooth appearance of the galaxy points towards it being at a reasonably high state of equilibrium.
