The galaxy appears as a moderately luminous object with a slightly elongated, but generally smooth, structure. The light profile seems to fall off gradually from the center. There is a hint of disk morphology, though the image resolution limits detailed characterization. The galaxy color seems moderately blue suggesting it is not a dormant, but it is likely a more passive system. Based on the smooth appearance and color, I suspect it has not undergone major mergers recently, though there might be indications of minor disturbance. The galaxy's stellar population is likely dominated by older stars, but with a small amount of ongoing star formation.
