The galaxy presents as a singular, somewhat elliptical object. Its color profile appears to be concentrated in the yellow-red spectrum, suggesting an older stellar population. A smaller, fainter, and more reddish secondary object is present within the same visual field as the main galaxy, though whether it is gravitationally bound or simply a projection effect is indeterminate from this image alone. The primary galaxy exhibits a smooth, fairly concentrated profile, with no obvious spiral arm structures or dust lanes. The galaxy displays a relatively high degree of roundness. The apparent lack of significant blue emission implies a suppressed rate of on-going star formation.
