The galaxy appears as a centrally concentrated, relatively smooth object. It exhibits a generally elliptical morphology, showing a high degree of roundness. The galaxy's color profile indicates the presence of both younger, bluer stellar populations, as well as older, redder populations; with an overall yellowish hue to the galaxy.  There is minimal visual evidence of significant ongoing star formation regions or prominent dust lanes.  Based on its morphology, it is unlikely that this is a spiral galaxy, or a galaxy undergoing a major merger.
