This galaxy presents as a generally smooth, elliptical-like structure. There is a concentrated, bright central bulge that graduates into a fainter halo. The color profile indicates an older stellar population, predominantly exhibiting redder hues. No distinct spiral arms or dust lanes are discernible at this resolution. There is only a slight blue tint in what may be the outer disk, but this is not well defined. It appears to be a relatively isolated system, showing no obvious signs of tidal disruption or interaction with neighboring galaxies.
