The galaxy presents as a fairly compact and well-defined object, roughly circular in shape. Its apparent size suggests a moderate physical extent, on the order of tens of thousands of light-years. The light distribution appears to be smoothly distributed and centrally concentrated. The galaxy's color is predominantly yellowish-orange, suggesting a stellar population dominated by older, redder stars, although there may be a small amount of star formation occuring. There is little evidence of spiral arms or a prominent disk. Some indication of minor disruption is apparent, although this galaxy does not seem to be undergoing a major merger event.
