The galaxy presents as a relatively smooth, elliptical-like structure. It appears largely featureless, with a concentrated, bright central bulge that gradually fades into the outer regions. The color profile is dominated by yellowish hues, indicative of an older stellar population. There is little evidence of spiral arms or dust lanes. There is a very slight suggestion of a disk shape, but the spheroid component is dominant. Given the morphology, this galaxy may be relatively massive, and exhibits very little ongoing star formation. There are no obvious signs of tidal disturbances or recent merger activity. The light profile suggests a smooth transition between the core and halo.
