The galaxy presents as a relatively smooth, elliptical structure. The light distribution suggests a central bulge with a gradual decrease in luminosity towards the outer regions. There may be a very faint, diffuse disk, but no prominent spiral arms or distinct features are readily apparent. The galaxy exhibits a color gradient, appearing yellower and more concentrated towards the center, potentially indicating an older stellar population with less ongoing star formation. The bluer, fainter outer regions may suggest the presence of younger stars or recent star-forming activity, but this is not strongly indicated. There is no clear evidence of significant tidal disturbances or interactions with other galaxies. The overall morphology suggests a galaxy that is likely in a relatively stable state.
