The galaxy appears to be a relatively bright, intermediate-redshift object. It exhibits a primarily smooth morphology, with a high likelihood of being elliptical, although there is a hint of a possible faint disk. The light profile is somewhat concentrated toward the center. The galaxy has a significant size, suggesting it is a massive system. There is no significant evidence of strong tidal features or ongoing major mergers, but a minor disturbance or merging could be occurring within the galaxy, or possibly at the fringes. There appears to be relatively little ongoing star formation, but there is still some. The light emitted appears to be strongest in redder wavelengths, and less in blue wavelengths. The galaxy is neither perfectly round, nor obviously elongated, and exhibits a shape that is somewhere in between.
